WO2010053106A1 - Perpendicular magnetic recording medium and magnetic storage device - Google Patents

Perpendicular magnetic recording medium and magnetic storage device Download PDF

Info

Publication number
WO2010053106A1
WO2010053106A1 PCT/JP2009/068866 JP2009068866W WO2010053106A1 WO 2010053106 A1 WO2010053106 A1 WO 2010053106A1 JP 2009068866 W JP2009068866 W JP 2009068866W WO 2010053106 A1 WO2010053106 A1 WO 2010053106A1
Authority
WO
WIPO (PCT)
Prior art keywords
layer
magnetic recording
metal layer
perpendicular magnetic
recording
Prior art date
Application number
PCT/JP2009/068866
Other languages
French (fr)
Japanese (ja)
Inventor
廣常朱美
Original Assignee
株式会社日立製作所
Priority date (The priority date is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the date listed.)
Filing date
Publication date
Application filed by 株式会社日立製作所 filed Critical 株式会社日立製作所
Publication of WO2010053106A1 publication Critical patent/WO2010053106A1/en

Links

Images

Classifications

    • GPHYSICS
    • G11INFORMATION STORAGE
    • G11BINFORMATION STORAGE BASED ON RELATIVE MOVEMENT BETWEEN RECORD CARRIER AND TRANSDUCER
    • G11B5/00Recording by magnetisation or demagnetisation of a record carrier; Reproducing by magnetic means; Record carriers therefor
    • G11B5/62Record carriers characterised by the selection of the material
    • G11B5/64Record carriers characterised by the selection of the material comprising only the magnetic material without bonding agent
    • G11B5/66Record carriers characterised by the selection of the material comprising only the magnetic material without bonding agent the record carriers consisting of several layers
    • G11B5/672Record carriers characterised by the selection of the material comprising only the magnetic material without bonding agent the record carriers consisting of several layers having different compositions in a plurality of magnetic layers, e.g. layer compositions having differing elemental components or differing proportions of elements
    • GPHYSICS
    • G11INFORMATION STORAGE
    • G11BINFORMATION STORAGE BASED ON RELATIVE MOVEMENT BETWEEN RECORD CARRIER AND TRANSDUCER
    • G11B5/00Recording by magnetisation or demagnetisation of a record carrier; Reproducing by magnetic means; Record carriers therefor
    • G11B5/62Record carriers characterised by the selection of the material
    • G11B5/73Base layers, i.e. all non-magnetic layers lying under a lowermost magnetic recording layer, e.g. including any non-magnetic layer in between a first magnetic recording layer and either an underlying substrate or a soft magnetic underlayer
    • G11B5/7368Non-polymeric layer under the lowermost magnetic recording layer
    • G11B5/7369Two or more non-magnetic underlayers, e.g. seed layers or barrier layers
    • GPHYSICS
    • G11INFORMATION STORAGE
    • G11BINFORMATION STORAGE BASED ON RELATIVE MOVEMENT BETWEEN RECORD CARRIER AND TRANSDUCER
    • G11B5/00Recording by magnetisation or demagnetisation of a record carrier; Reproducing by magnetic means; Record carriers therefor
    • G11B5/74Record carriers characterised by the form, e.g. sheet shaped to wrap around a drum
    • G11B5/82Disk carriers

Definitions

  • the present invention relates to an energy-assisted perpendicular magnetic recording medium and a magnetic storage device.
  • the surface recording density of a magnetic disk device has become several hundred Gbit / inch 2 or more, and the recording system has changed from the in-plane magnetic recording system to the perpendicular magnetic recording system as the density increases.
  • This method has been found to be more effective for higher density than in-plane magnetic recording because the leakage flux from adjacent bits works in a direction to stabilize the magnetization when performing high-density recording.
  • it is necessary to solve the problem of the stability against the environmental temperature, that is, the thermal demagnetization phenomenon even when the bit is reduced.
  • the energy assist method using near-field light can make the light spot extremely small in size below the wavelength as compared with a method of forming a diaphragm light spot with a laser beam using a lens or the like. For this reason, energy can be locally irradiated in a very narrow range with a diameter of a region heated by energy assist of several + nm or less, and it is considered suitable for high density recording of 1 Tbit / inch 2 or more (Non-patent Document 1). ).
  • the energy assist method using near-field light has a characteristic that the intensity of the near-field light rapidly decreases with respect to the distance from the light source, so when the recording layer exists at a distance away from the light source, The intensity of light applied to the recording layer is reduced, and there is a problem that the recording layer cannot be heated practically. Further, when the magnetic spacing is reduced by bringing the recording layer close to the light source, the flying characteristics of the head are not stable. Furthermore, a recording layer having a large perpendicular magnetic anisotropy energy and coercive force at room temperature has a high Curie temperature, and irreversible deterioration occurs in the protective layer, the recording layer, etc. when the energy is irradiated many times up to the recording temperature. Therefore, it is difficult to record many times. The recording layer having a low Curie temperature has a problem that the perpendicular magnetic anisotropy energy and the coercive force are too small.
  • the recording layer cannot be heated practically enough for energy assist using near-field light.
  • the recording layer cannot be heated practically enough for energy assist using near-field light.
  • An object of the present invention is to provide a perpendicular magnetic recording medium and a magnetic storage device that can solve the above-described problems and realize high-density energy-assisted perpendicular magnetic recording.
  • a perpendicular magnetic recording medium that performs recording in a state where anisotropy is reduced wherein an intermediate layer is made of Ru and / or Pd, and the magnetic recording layer is mainly composed of a ferromagnetic metal layer mainly composed of Co and Pd.
  • the film thickness of the ferromagnetic metal layer is 0.15 or more and 0.25 nm or less, and the film thickness of the nonmagnetic metal layer is 0.45 or more and 0.8 nm or less.
  • the film thickness ratio between the ferromagnetic metal layer and the nonmagnetic metal layer is 2 or more and 4 or less, and the difference in coercive force between energy irradiation and non-irradiation is 8 kOe or more.
  • a non-magnetic metal layer as a component, and the cap layer is composed of a ferromagnetic metal layer mainly composed of Co and a non-magnetic metal layer mainly composed of Pd.
  • the difference in coercive force between time and non-irradiation is 8 kOe or more It was.
  • the Curie temperature of the magnetic recording layer is 220 ° C. or higher and 400 ° C. or lower.
  • the perpendicular magnetic recording medium according to (1) or (2) is characterized in that the average oxygen concentration in the magnetic recording layer is 5 atomic% or more and 15 atomic% or less.
  • the perpendicular magnetic recording medium according to (1) or (2) is characterized in that the average boron concentration in the ferromagnetic metal layer is 5 atomic% or more and 15 atomic% or less.
  • the thickness of the magnetic recording layer is 6 nm or more and 15 nm or less.
  • the perpendicular magnetic recording medium according to (2) is characterized in that the average oxygen concentration in the cap layer is lower than the average oxygen concentration in the magnetic recording layer.
  • the cap layer has a thickness of 1 nm to 4 nm.
  • the intermediate layer according to (1) or (2) is characterized by being made of Pd.
  • the intermediate layer according to (1) or (2) is characterized by being made of Ru.
  • the intermediate layer described in (1) or (2) is characterized by being made of Ru and Pd.
  • a magnetic storage device comprising: a perpendicular magnetic recording medium for recording in a state of reduced performance; a magnetic recording head having an energy irradiation function using near-field light; and a magnetic head having a signal reproducing head.
  • the intermediate layer is made of Ru and / or Pd
  • the magnetic recording layer is a laminate of a ferromagnetic metal layer mainly containing Co and a nonmagnetic metal layer mainly containing Pd.
  • the film thickness of the ferromagnetic metal layer is 0.15 nm or more and 0.25 nm or less
  • the film thickness of the nonmagnetic metal layer is 0.45 nm or more and 0.8 nm or less
  • the film of the ferromagnetic metal layer and the nonmagnetic metal layer The thickness ratio is 2 or more and 4 or less
  • energy The difference in coercivity at and during non-irradiation morphism There are more than 8 kOe, the distance from the energy radiation source of the magnetic head during recording to the magnetic recording layer surface of the perpendicular magnetic recording medium is characterized in that it is 8nm or less.
  • a perpendicular magnetic recording medium and a magnetic storage device suitable for high-density heat-assisted recording capable of recording at a temperature rise by heat assist, and having a high coercive force at room temperature.
  • FIG. 1 is a schematic cross-sectional view showing the overall layer configuration of a perpendicular magnetic recording medium of the present invention.
  • FIG. 3 is a diagram showing a detailed cross-sectional structure of an intermediate layer and a recording layer of a perpendicular magnetic recording medium according to the present invention, and shows a state in which the intermediate layer is laminated.
  • FIG. 3 is a diagram showing a detailed cross-sectional structure of the intermediate layer and the recording layer of the perpendicular magnetic recording medium of the present invention, and shows a state in which the recording layer is laminated on the intermediate layer.
  • the expanded sectional view of a recording layer is a diagram showing a detailed cross-sectional structure of an intermediate layer and a recording layer of a perpendicular magnetic recording medium according to the present invention, and shows a state in which the intermediate layer is laminated.
  • the figure which shows the relationship between the ferromagnetic metal layer film thickness, a floating characteristic, and a magnetic characteristic in the perpendicular magnetic recording medium of this invention The figure which shows the relationship between the film thickness of a nonmagnetic metal layer, a temperature characteristic, and a magnetic characteristic in the perpendicular magnetic recording medium of this invention.
  • FIG. 2 is a schematic cross-sectional view showing the entire layer structure of a perpendicular magnetic recording medium having a cap layer of the present invention. The enlarged view of a cap layer.
  • FIG. 12A is a cross-sectional view taken along the line A-A ′ of FIG. 12A.
  • 1 is a schematic view of a head mounted on a magnetic storage device of the present invention. Schematic view seen from the side of the main part of the head.
  • a perpendicular magnetic recording medium having a magnetic recording layer having perpendicular magnetic anisotropy at room temperature and performing recording in a state where the perpendicular magnetic anisotropy is reduced by energy irradiation (assist) is provided.
  • energy assist was performed using near-field light.
  • energy can be locally irradiated in a very narrow range in which the diameter of the heated region in the medium is several + nm or less.
  • the energy dose was optimized and evaluated so that the temperature of the medium was about 70% or more of the Curie point.
  • FIG. 1A schematically shows a cross-sectional structure of a perpendicular magnetic recording medium having a recording layer 104 composed of a multilayer film of a ferromagnetic metal layer 108 and a nonmagnetic metal layer 109 as one embodiment of the present invention. It is. On the substrate 101, a Ni 63 Ta 38 layer of about 30 nm and a Ni 94 W 6 layer of about 7 nm as the underlayer 102, a Ru layer of about 16 nm as the intermediate layer 103, a recording layer 104 of about 12 nm, and a protective layer 106 of about 3 nm CN layers were sequentially formed. Film formation was performed by DC sputtering.
  • FIG. 1B is an enlarged conceptual diagram of the recording layer 104.
  • Co 90 B 10 was used for the ferromagnetic metal layer 108
  • Pd was used for the nonmagnetic metal layer 109.
  • the multilayer film was formed by alternately forming both layers while fixing the substrate and rotating the Co 90 B 10 target and the Pd target using a rotating cathode, and formed a total film of about 12 nm.
  • the ferromagnetic metal layer 108 and the nonmagnetic metal layer 109 are alternately laminated 15 times as the constituent layers by 0.2 nm and 0.6 nm, respectively. Yes. Since the origin of perpendicular magnetic anisotropy in the case of a multilayer film is mainly the interface, it is important that the two layers are alternately stacked to form an interface, and a ferromagnetic metal layer and a nonmagnetic metal layer Either of these may be formed first.
  • a similar multilayer film can be formed by fixing the target and rotating the substrate. The film thickness of each constituent layer was changed by changing the power input to each target. Further, in order to form a grain boundary structure in the multilayer recording layer, a small amount of oxygen was added during film formation.
  • the intermediate layer 103 is formed with 8 nm of Ru as the first intermediate layer 201 at a low gas pressure (1.4 Pa), and then 8 nm of Ru as the second intermediate layer 202 at a high gas pressure (5 Pa). Formed.
  • a flat film is formed at a low gas pressure to adjust the crystallinity, and a film is formed thereon at a high gas pressure to form a concavo-convex shape (FIG. 2A).
  • a multilayer recording layer 104 having good crystal orientation in the vertical direction can be formed on the shape in which the grains are separated (FIG. 2B).
  • the multilayer film of the ferromagnetic metal layer 108 and the nonmagnetic metal layer 109 is mainly formed in the crystal grains 203 (FIG. 2C).
  • the range of gas pressure during intermediate layer deposition when the low gas pressure is 1 to 2 Pa and the high gas pressure is 4 to 10 Pa, the uneven shape is formed, and the separation of the recording layer is promoted and the crystal orientation is improved. The effect to do was obtained.
  • the thickness of the nonmagnetic metal layer was kept constant at 0.6 nm, and the floating characteristics of the ferromagnetic metal layer and the thickness dependence of the saturation magnetization were investigated. The results are shown in FIG.
  • the number of constituent layers is 18 to 12, but since the magnetic moment is proportional to the recording layer thickness, the total thickness of the recording layer was constant at about 12 nm.
  • the flying characteristics were measured by plotting the output of the piezoelectric terminal vibration when the head floated with a tester having a magnetic head with a dedicated piezoelectric sensor terminal attached to the head. The flatter the lubricant surface of the medium and the more stable the head flies without colliding with the medium, the smaller the output, and the smaller the output. When the levitation is stable, the piezo output is 31.5 mV or less, and the vibration becomes larger as the levitation becomes unstable, such as hitting or colliding, and the output increases.
  • the piezo output is 31.5 mV or less. Furthermore, 31.4 mV or less is more preferable because it is a level at which the medium and the head do not collide even when a disturbance such as external vibration occurs.
  • the saturation magnetization was measured using a vibrating magnetic magnetometer (VSM) after the medium was cut into small pieces. In the present specification, evaluations not particularly described in temperature were all performed at room temperature. If the saturation magnetization is small, the signal level when the bit is recorded becomes low, the SNR becomes low, and the correctly recorded information cannot be reproduced. For this reason, it is important that the saturation magnetization is 290 emu / cc or more.
  • the thinner the ferromagnetic metal layer the smaller the piezo output at the time of flying the head, and the better the flying characteristics, and the thicker the saturation magnetization becomes.
  • the piezoelectric output is 31.5 mV or less and the saturation magnetization is 290 emu / cc or more. It was.
  • the piezo output is 31.4 mV or less
  • the saturation magnetization is 310 emu / cc or more, and both the floating characteristics and the magnetic characteristics are better. Results were obtained.
  • the film thickness of the ferromagnetic metal layer was kept constant at 0.2 nm, and the dependence of the temperature characteristics and saturation magnetization on the film thickness of the nonmagnetic metal layer was investigated. The results are shown in FIG.
  • Nonmagnetic metal layer thickness (nm) Saturation magnetization (emu / cc) Curie temperature (° C) 1.0 210 150 0.8 296 220 0.7 310 280 0.6 336 320 0.5-370 0.45 385 400 0.4 405 420 0.3 425-
  • the number of constituent layers is 10 to 24, but since the magnetic moment is proportional to the thickness of the recording layer, the total thickness of the recording layer was kept constant at about 12 nm.
  • the temperature characteristics were obtained by measuring the saturation magnetization at each temperature while heating with a heater after cutting the medium into small pieces, and the temperature at which the saturation magnetization was sufficiently small at 20 emu / cc or less was taken as the Curie temperature. In the method of recording by reducing the perpendicular magnetic anisotropy by energy irradiation, the temperature characteristic is also an important physical property. When the Curie temperature is too low, the saturation magnetization is lowered by a small amount of energy irradiation, so that it is difficult to control the energy irradiation amount.
  • the Curie temperature is preferably 400 ° C. or lower.
  • the saturation magnetization increases as the film thickness of the nonmagnetic metal layer decreases, and the Curie temperature decreases as the film thickness increases.
  • the Curie temperature is 400 ° C. or less and the saturation magnetization is 290 emu / cc or more. It was.
  • the saturation magnetization is 310 emu / cc or more, and both the temperature characteristics and the magnetic characteristics are better. was gotten.
  • FIG. 5 and Table 3 show the results of examining the magnetic characteristics while changing the film thickness ratio between the nonmagnetic metal layer and the ferromagnetic metal layer.
  • the coercive force was examined using a Kerr effect measuring device. If the coercive force is low, an unstable region of the recorded region disappears due to a head magnetic field, a rise in the temperature around the head, or the like. . From FIG. 5 and Table 3, it can be seen that the coercive force increases when the film thickness ratio between the nonmagnetic metal layer and the ferromagnetic metal layer is in an appropriate range. When the film thickness ratio between the nonmagnetic metal layer and the ferromagnetic metal layer was 2 or more and 4 or less, a coercive force of 9 kOe or more was obtained. Furthermore, when the film thickness ratio between the nonmagnetic metal layer and the ferromagnetic metal layer was 2.5 or more and 3.5 or less, a better result was obtained with a coercive force of 10.5 kOe or more.
  • Table 4 shows a result of comparing the case where the film thickness ratio is constant and the film thickness of the magnetic metal layer and the ferromagnetic metal layer is within the above-mentioned preferable range and the case outside the range.
  • the film thickness ratio between the nonmagnetic metal layer and the ferromagnetic metal layer is in an appropriate range
  • the film thickness of the constituent layer is out of the appropriate range (numbers 41, 43, 44), that is, here
  • the thickness of the ferromagnetic metal layer is 0.4, 0.1, 0.08 nm
  • the coercive force is smaller than 9 kOe.
  • Fig. 6 and Table 5 show the results of examining the relationship between the difference in coercive force during energy irradiation and non-irradiation and the signal degradation amount.
  • the energy light source wavelength during recording was 780 nm
  • the emission power of the energy light source was 100 mW
  • the energy irradiation time was 2 ns
  • the recording magnetic field was about 6 kOe
  • the medium shown in FIG. 1 was used.
  • the measurement was performed according to the following procedure. After recording with energy assist at a linear recording density of 1500 fci, the signal level was measured. Next, recording was performed on the adjacent tracks at a linear recording density of 1000 fci, and the level of the signal recorded first was measured again. When recording on the tracks on both sides, the already recorded track is also exposed to the head magnetic field and temperature rise leaked from the adjacent track.
  • the signal degradation amount was calculated as the signal degradation amount by the difference in signal level between the first recording and the recording on both sides.
  • the ferromagnetic metal layer thickness is 0.2 nm
  • the non-magnetic metal layer thickness is 0.6 nm
  • the total recording layer thickness is 12 nm
  • the combination of the intermediate layer material and the film forming process is changed.
  • the magnetic force was examined.
  • a comparison was also made between the case where the intermediate layer was formed by the low gas pressure and high gas pressure film forming processes and the case where the intermediate layer was formed by a single film forming process. Table 6 summarizes the results.
  • the intermediate layer material was Ru and / or Pd
  • a large coercive force of 9 kOe was obtained.
  • the coercive force was as small as 4 to 6 kOe when the intermediate layer material was other than Ru and Pd, or when the intermediate layer was not formed.
  • the intermediate layer is a single layer, the coercive force is low because the crystal grains are not sufficiently separated.
  • Ru has good characteristics because the hcp structure crystal improves the c-axis of the Co layer or the (111) orientation of the Pd layer, and forms an uneven shape. This is probably because the perpendicular magnetic anisotropy of the recording layer is easily formed.
  • Co having the same hcp structure has little formation of uneven shapes and a good coercive force could not be obtained.
  • Pd has an fcc structure, it is considered that the coercive force is increased because the uneven shape is large and the separation of crystal grains is promoted.
  • mass production can be improved by using Pd for film formation at a high gas pressure.
  • the surface roughness was large, the roughness of number 61 was 1.5 times that of number 63, and number 62 was 1.3 times that of number 63.
  • the magnetic recording layer As described above, it has a substrate, an underlayer and an intermediate layer provided on the substrate, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature, and a protective layer, and the perpendicular magnetic anisotropy is reduced by energy irradiation.
  • an intermediate layer is formed of Ru and / or Pd
  • the magnetic recording layer includes a ferromagnetic metal layer mainly containing Co and a nonmagnetic metal layer mainly containing Pd.
  • the ferromagnetic metal layer has a thickness of 0.15 nm to 0.25 nm and the nonmagnetic metal layer has a thickness of 0.45 nm to 0.8 nm.
  • tempered glass having a diameter of 2.5 inches, a thickness of 0.6 mm, and a surface roughness Ra of 0.3 nm or less was used, but the diameter was 3.5 inches, 5 inches, or 1.8 inches.
  • a substrate having a different size such as 1 mm, 0.8 mm, or 0.5 mm may be used.
  • the material of the substrate may be other than tempered glass, but a material such as Si or aluminum that does not deform or change even when the surface is exposed to about 500 ° C. is preferable.
  • the protective layer 106 may have a different composition ratio or other materials as long as adhesion to the recording layer, transparency at the wavelength of the heat-assisted light source, and surface flatness can be ensured.
  • the film thickness of the ferromagnetic metal layer is 0.2 nm
  • the film thickness of the nonmagnetic metal layer is 0.6 nm
  • the total film thickness of the recording layer is 12 nm
  • the amount of oxygen added to the Ar gas during film formation is changed.
  • the oxygen amount was analyzed using an energy dispersive X-ray analyzer (EDX).
  • EDX energy dispersive X-ray analyzer
  • the crystal orientation was examined using an X-ray diffractometer. The better the crystal orientation, the more uniform the magnetic properties of each crystal. When the crystal orientation deteriorates, the dispersion of magnetic characteristics increases and causes noise. Therefore, the crystal orientation is preferably 3.35 ° or less.
  • the grain boundary width was determined by observing 100 grains and grain boundaries with a transmission electron microscope (TEM), and obtaining an average value of the grain boundaries. The larger the grain boundary width, the less magnetic influence of adjacent particles. That is, the magnetic correlation distance is reduced and the recording error rate is reduced. Therefore, the crystal grain boundary needs to be large, and is preferably at least 0.3 nm or more. When the grain boundary is not formed, the magnetic correlation distance is too large, and a high-density bit such as a bit length of 25 nm cannot be formed.
  • the crystal orientation deteriorates and the grain boundary width increases as the amount of oxygen increases.
  • the amount of oxygen in the recording layer was 5 atom% or more and 15 atom% or less
  • the crystal orientation was 3.35 ° or less and the grain boundary width was 0.3 nm or more, and good results were obtained.
  • the oxygen content in the recording layer is 8 atomic% or more and 13 atomic% or less
  • the crystal orientation can be 3.3 ° or less and the grain boundary width can be 0.4 nm or more, and a better result is obtained. .
  • the crystal grain size by adding B (boron) into the ferromagnetic metal layer.
  • B boron
  • 100 particles were observed with a transmission electron microscope (TEM), and the average value and dispersion of the grain size were obtained.
  • TEM transmission electron microscope
  • the average grain size is preferably 11.4 nm or less.
  • the heating time of the medium during actual recording is several ns, the deterioration of the saturation magnetization when heated at 400 ° C. for 1 h was examined as an acceleration test.
  • the amount of deterioration is large, the number of rewritable times decreases, and therefore it is preferably 200 emu / cc or less.
  • Prepare targets with different boron (B) contents in the ferromagnetic metal layer the ferromagnetic metal layer thickness is 0.2 nm, the nonmagnetic metal layer thickness is 0.6 nm, and the total recording layer thickness is 12 nm.
  • B boron
  • Table 8 Number Boron amount Saturation magnetization deterioration Crystal grain size (Atom%) (emu / cc) (nm) 81 0 20 12.5 82 5 20 11.0 83 8 30 10.8 84 10 50 10.6 85 13 100 10.5 86 15 180 10.3 87 19 250 10.2
  • the saturation magnetization deterioration amount can be 200 emu / cc or less, the crystal grain size could be 11 nm or less, and good results were obtained.
  • the saturation magnetization deterioration amount can be 100 emu / cc or less and the crystal grain size can be 10.8 nm or less, and a better result is obtained.
  • the relationship between the Curie temperature of the recording layer, the flying characteristics, and the recording characteristics was examined.
  • the flying characteristics an acceleration test was conducted, and the number of times the glide head hits when flying with the glide tester after irradiating the medium with far-field laser light (wavelength 780 nm, spot diameter 1 ⁇ m) 10 ns for 1000 times.
  • the recording characteristics recording was performed with near-field light at a bit length of 50 nm, and 100 recording domains were observed with a magnetic microscope (MFM) to determine the bit length dispersion. The measurement was compared with the dispersion at the optimum power of each medium while changing the recording power. Table 9 summarizes the results.
  • the higher the Curie temperature of the recording layer the greater the number of head hits. This is because, since the Curie temperature is high, recording cannot be performed unless the temperature of the recording layer is increased during recording, and the protective layer and the lubricant are thermally deteriorated by the heat at this time. It is considered that irregularities are formed on the surface, the floating characteristics are deteriorated, and the number of hits is increased. Further, the lower the Curie temperature of the recording layer, the larger the bit length dispersion. This is because the temperature at the time of recording is low, that is, the output power is low and the difference from room temperature is small, so that the variation in temperature control increases. When the recording layer Curie temperature was 220 ° C. or higher and 400 ° C.
  • the number of head hits was as small as 5 or less, and good results were obtained with a bit length dispersion of 15% or less. Further, when the recording layer Curie temperature was 250 ° C. or higher and 370 ° C. or lower, the number of hits of the head was very small, 2 times or less, and a better result was obtained with a bit length dispersion of 10% or less.
  • the relationship between the film thickness of the recording layer, temperature characteristics, and magnetic characteristics was examined.
  • the results are shown in Table 10.
  • the temperature characteristics the temperature difference between the energy incident side (upper surface) of the recording layer and the opposite substrate side (lower surface) was examined.
  • the temperature difference is large, when the recording layer is irradiated with energy for recording, the perpendicular magnetic anisotropy is decreased by heating only the upper surface and the magnetization is reversed, but the lower surface remains low in temperature and high in perpendicular magnetic anisotropy. For this reason, magnetization reversal does not occur, and the rate at which recording bits are not formed increases. Therefore, the temperature difference between the upper and lower recording layers is preferably 125 ° C.
  • the magnitude of the magnetic moment is shown as a ratio with the nominal recording layer 12 nm being 1.
  • the magnitude of the magnetic moment needs to be 0.5 or more of the nominal value.
  • Table 10 shows that the temperature difference between the upper and lower recording layers increases as the recording layer thickness increases. This is because the light intensity decreases where the near-field light is separated from the light source.
  • the magnetic moment decreases as the recording layer thickness decreases. This is because it is related to the magnetization of the recording layer and its volume.
  • the thickness of the recording layer was 6 nm or more and 15 nm or less, good results were obtained in which the temperature difference between the upper and lower recording layers was 125 ° C. and the magnetic moment was 0.5 or more.
  • the recording layer thickness was 8.4 nm or more and 13 nm or less, a better result was obtained in which the temperature difference between the upper and lower recording layers was 105 ° C. and the magnetic moment was 0.7 or more.
  • Example 2 As one example of the present invention, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature and a cap layer are provided, and the perpendicular magnetic anisotropy is lowered by energy irradiation (assist). A perpendicular magnetic recording medium for recording will be described.
  • FIG. 9A shows a recording layer 104 composed of a multilayer film of a ferromagnetic metal layer 108 and a nonmagnetic metal layer 109, a cap layer ferromagnetic metal layer 901, and a cap layer nonmagnetic as an embodiment of the present invention.
  • 1 schematically shows a cross-sectional structure of a perpendicular magnetic recording medium having a cap layer 105 formed of a multilayer film of metal layers 902.
  • a Ni 63 Ta 38 layer and a Ni 94 W 6 layer of about 30 nm as the underlayer 102, a Ru layer of about 16 nm as the intermediate layer 103, a recording layer 104 of about 12 nm, and a cap layer 105 of about 3 nm.
  • a CN layer of about 3 nm was sequentially formed as the protective layer 106. Film formation was performed by DC sputtering. Thereafter, about 107 nm of the lubricant 107 was applied on the CN layer.
  • the recording layer 104 was laminated using Co 90 B 10 of 0.2 nm for the ferromagnetic metal layer 108 and Pd of 0.6 nm for the nonmagnetic metal layer 109, and a trace amount of oxygen was added. Details are as described in Example 1.
  • FIG. 9B is an enlarged view of the cap layer 105.
  • the cap layer 105 was laminated by using 0.2 nm of Co for the ferromagnetic metal layer 901 for the cap layer and 0.6 nm of Pd for the nonmagnetic metal layer 902 for the cap layer. When the cap layer is 3 nm, the number of layers is about 4 times.
  • the cap layer having the multilayer structure was formed by alternately forming both layers while fixing the substrate and rotating the Co target and the Pd target. A similar multilayer film can be formed by fixing the target and rotating the substrate. The film thickness of each constituent layer was changed by changing the power input to each target.
  • the gas pressure during cap layer deposition was 5 Pa.
  • a medium having a multi-layered cap layer and a comparative cap layer was formed, and the flying characteristics of the perpendicular magnetic recording medium were examined and compared in Table 11.
  • the yield at which a medium with good flying characteristics was obtained was examined.
  • 20 media having the same configuration were prepared, and those with a piezoelectric output of 31.3 mV or less were Class A products, those with 31.4 to 31.5 mV were Class B products, and those with 31.6 mV or more were used. Each percentage was examined by counting as NG.
  • the thicker the cap layer the higher the yield.
  • the A-class product yield was 90%, and good results were obtained.
  • the cap layer thickness was 2 nm or more, the yield of Class A products was improved to 95%, and better results were obtained.
  • the improvement of the flying characteristics was similarly improved in both the multilayer cap layer and the comparative cap layer. The reason why the flying characteristics are improved is considered to be that the unevenness formed by the formation of crystal grains on the surface of the recording layer was made smooth by forming the cap layer 105 as shown in FIG.
  • the magnetic characteristics were compared.
  • the coercive force of each medium was measured, and the amount of coercive force deterioration due to cap layer formation was examined.
  • the magnetic characteristics when the cap layer is formed in the present invention and the comparative example are compared in FIG.
  • the comparative example having a Co 65 Cr 15 Pt 12 B 8 composition cap layer that is not multi-layered the coercive force deterioration was extremely large, and even when 1 nm was formed, a large deterioration of 2 kOe or more was shown. This is because the cap layer having a small coercive force was formed on the recording layer having a large coercive force, so that the magnetic characteristics of the entire medium deteriorated.
  • the medium with a multilayer film cap layer of the present invention even if a cap layer is formed to improve the floating characteristics, the deterioration of magnetic characteristics is extremely small, and even if a 4 nm cap layer is formed, the deterioration is as small as 1.5 kOe. I understand that. This is presumably because the cap layer also has a multilayer film structure so that layers having a large coercive force are stacked.
  • a cap layer having a multilayer structure comprising a ferromagnetic metal layer for a cap layer and a nonmagnetic metal layer for a cap layer on a recording layer having a high perpendicular magnetic anisotropy, it is possible to prevent deterioration of magnetic characteristics and As a result, the flying characteristics can be made extremely good.
  • composition and process dependency of the multilayer cap layer were investigated while keeping the conditions of the recording layer, etc., and are shown in Table 12.
  • a medium in which Co 90 B 10 is 0.2 nm for the ferromagnetic metal layer 901 for the cap layer and Pd is 0.6 nm for the nonmagnetic metal layer 902 for the cap layer was manufactured (No. 121).
  • the thickness of the cap layer was 2 nm.
  • a medium in which the ferromagnetic metal layer 901 for the cap layer was laminated using Co of 0.2 nm and the nonmagnetic metal layer 902 for the cap layer was laminated using 0.6 nm of Pd was produced.
  • a small amount of oxygen was added.
  • the amount of O in the cap layer was 10 atomic% (No. 122)
  • the yield of the class A product decreased to 80%.
  • the amount of O in the cap layer was 5 atomic% (No. 123)
  • the yield of the class A product was 85%. From this, it was found that a smaller amount of oxygen in the cap layer is better.
  • a medium (No. 124) was prepared by laminating Co 90 B 10 with 0.1 nm for the cap layer ferromagnetic metal layer 901 and Pd with 0.6 nm for the non-magnetic metal layer 902 for cap layer.
  • the thickness of the cap layer was 2 nm. It has been found that when such a ferromagnetic metal layer is made thinner than the recording layer, the degradation of the coercive force can be reduced while the yield of the class A product remains 95%.
  • a medium (No. 125) was prepared by laminating Co for the cap layer ferromagnetic metal layer 901 with 0.1 nm of Co and for the cap layer nonmagnetic metal layer 902 with Pd of 0.6 nm.
  • the thickness of the cap layer was 2 nm.
  • a medium (No. 127) in which Co is 0.2 nm for the ferromagnetic metal layer 901 for the cap layer, Pd is 0.6 nm for the nonmagnetic metal layer 902 for the cap layer, and the sputtering gas pressure is 3.5 Pa.
  • the thickness of the cap layer was 2 nm.
  • the gas pressure is lowered in this way, the film forming rate is increased and the mass productivity is improved.
  • the yield of Class A products improved to 97%.
  • the degradation of the coercive force was slightly increased.
  • Example 1 The layer configuration, manufacturing method, material, evaluation method, etc. not described in this example were the same as in Example 1.
  • FIG. (A) is a schematic plan view, and (b) is an AA ′ sectional view thereof.
  • (C) is a schematic diagram of the head, and (d) is a schematic diagram viewed from the side of the main part of the head.
  • This apparatus has a perpendicular magnetic recording medium 1501, a driving unit 1502 for driving the medium 150, a magnetic head flying slider 1503, a magnetic head driving means 1504, and a magnetic head recording / reproducing signal processing means 1505.
  • the magnetic head is a recording / reproducing separation type magnetic head formed on a magnetic head slider.
  • the recording head is provided with means 1507 for forming a magnetic field and energy irradiation means 1506 using near-field light. Further, the magnetic head is provided with a reproducing current detecting means (reproducing head) 1508 to reproduce the recorded bit.
  • Near-field light is supplied to an energy irradiation means 1506 using near-field light through an optical waveguide 1202 formed on the suspension 1201.
  • the flying slider 1503 is attached to the suspension via the flexure 1203 in order to improve positioning accuracy.
  • the light source wavelength is 780 nm
  • the perpendicular magnetic recording medium 1501 has the structure shown in FIG. FIG. 13 shows the relationship between the distance (magnetic spacing) from the near-field light source, which is the energy irradiation source, to the recording layer surface and the energy absorption rate in the perpendicular magnetic recording medium. This was calculated from the intensity of near-field light and the absorptance of the medium at that wavelength, and normalized when the distance was 4 nm. From this, it can be seen that the smaller the distance, the larger the absorption rate of the medium. When the absorptance is small, the medium cannot be heated sufficiently with near-field light and recording cannot be performed.
  • the absorptance is preferably 25% or more.
  • the distance from the energy irradiation source to the recording layer surface was 8 nm or less, an absorptivity of 25% or more was obtained.
  • an absorptivity was 32% or more and a better result was obtained.
  • Example 2 After incorporating the medium described in Example 1 into the magnetic storage device and confirming that the head stably floats at a head flying height of 4 nm, a head equipped with the energy irradiation means using the near-field light is mounted. And recorded. When the domain was evaluated by MFM, it was found that a domain having a linear density direction of about 25 nm and a track width direction of 50 nm could be formed.
  • the substrate has a substrate, an underlayer and an intermediate layer provided on the substrate, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature, and a protective layer, and the perpendicular magnetic anisotropy is lowered by energy irradiation.
  • a perpendicular magnetic recording medium for recording in a state an intermediate layer is formed of Ru and / or Pd, and a magnetic recording layer is composed of a ferromagnetic metal layer mainly containing Co and a nonmagnetic metal layer mainly containing Pd.
  • the ferromagnetic metal layer has a thickness of 0.15 nm to 0.25 nm
  • the nonmagnetic metal layer has a thickness of 0.45 nm to 0.8 nm
  • the ferromagnetic metal layer is nonmagnetic.
  • a magnetic layer having a metal layer thickness ratio of 2 to 4 and a perpendicular magnetic recording medium in which the difference in coercivity between energy irradiation and non-irradiation is 8 kOe or more, and further has an energy irradiation function using near-field light. Includes a recording head and a signal playback head , The distance from the energy radiation source during recording to the magnetic recording layer surface by a 8nm or less, it is possible to obtain an energy-assisted magnetic memory device having good recording and reproduction characteristics.

Abstract

Provided is a medium that has high perpendicular magnetic anisotropy energy and high coercivity at room temperature, that has a low Curie temperature, and that enables recording even at low power with the perpendicular magnetic anisotropy energy and coercivity lowered. The perpendicular magnetic recording medium comprises a ground layer (102) and an intermediate layer (103) provided on a substrate (101) and a magnetic recording layer (104) that has perpendicular magnetic anisotropy at room temperature, and provides recording with the perpendicular magnetic anisotropy of the magnetic recording layer lowered by irradiation with energy. The intermediate layer comprises Ru and/or Pd. The magnetic recording layer is a laminate of a ferromagnetic metal layer (108) having Co as the principal component and a nonmagnetic metal layer (109) having Pd as the principal component. The ferromagnetic metal layer is from 0.15‑0.25 nm thick, the nonmagnetic metal layer is from 0.45‑0.8 nm thick, the thickness ratio of the ferromagnetic metal layer and the nonmagnetic metal layer is from 2‑4, and the difference in magnetic coercivity with energy irradiation and without irradiation is at least 8 kOe.

Description

垂直磁気記録媒体及び磁気記憶装置Perpendicular magnetic recording medium and magnetic storage device
 本発明は、エネルギーアシスト型垂直磁気記録媒体及び磁気記憶装置に関する。 The present invention relates to an energy-assisted perpendicular magnetic recording medium and a magnetic storage device.
 2008年現在、磁気ディスク装置(HDD)の面記録密度は数百Gbit/inch2以上となり、高密度化に伴い、面内磁気記録方式から垂直磁気記録方式へ記録方式が変化してきた。この方式では、高密度記録を行った際に、隣接ビットからの漏洩磁束が磁化を安定化させる方向に働くため、面内磁気記録と比べて、高密度化に有効であることがわかっている。しかしながら、1Tbit/inch2以上に高密度化するためには、ビットを小さくした場合でも環境温度に対する安定性つまり熱減磁現象の問題を解決する必要がある。 As of 2008, the surface recording density of a magnetic disk device (HDD) has become several hundred Gbit / inch 2 or more, and the recording system has changed from the in-plane magnetic recording system to the perpendicular magnetic recording system as the density increases. This method has been found to be more effective for higher density than in-plane magnetic recording because the leakage flux from adjacent bits works in a direction to stabilize the magnetization when performing high-density recording. . However, in order to increase the density to 1 Tbit / inch 2 or more, it is necessary to solve the problem of the stability against the environmental temperature, that is, the thermal demagnetization phenomenon even when the bit is reduced.
 この問題を解決するには、室温でさらに大きな垂直磁気異方性エネルギーや保磁力を有する記録層を適用する必要があるが、高保磁力の記録層に記録を行うことが出来るような、巨大な磁界を発生する記録磁気ヘッドの実現は非常に困難である。そこで、光照射により熱を発生させる等のエネルギーアシストにより、記録時のみ垂直磁気異方性エネルギーや保磁力を低下させて磁化反転を起こして記録を行い、それ以外のときには垂直磁気異方性エネルギーや保磁力を高いままにする、という画期的な記録方式が検討され始めた。中でも、近接場光を用いてエネルギーアシストする方式は、レーザ光をレンズ等で絞り光スポットを形成する方式に比べ、光スポットを波長以下の極めて小さいサイズに出来る。このためエネルギーアシストにより加熱される領域の直径が数+nm以下と非常に狭い範囲に局所的にエネルギー照射出来、1Tbit/inch2以上の高録密度記録に適していると考えられる(非特許文献1)。 In order to solve this problem, it is necessary to apply a recording layer having larger perpendicular magnetic anisotropy energy and coercive force at room temperature. Realization of a recording magnetic head that generates a magnetic field is very difficult. Therefore, recording is performed by lowering the perpendicular magnetic anisotropy energy and coercive force to cause magnetization reversal only during recording by energy assist such as generating heat by light irradiation, and at other times perpendicular magnetic anisotropy energy The groundbreaking recording method that keeps the coercive force high was started. In particular, the energy assist method using near-field light can make the light spot extremely small in size below the wavelength as compared with a method of forming a diaphragm light spot with a laser beam using a lens or the like. For this reason, energy can be locally irradiated in a very narrow range with a diameter of a region heated by energy assist of several + nm or less, and it is considered suitable for high density recording of 1 Tbit / inch 2 or more (Non-patent Document 1). ).
 一方で、近接場光を用いたエネルギーアシスト方式では、近接場光の強度が光源からの距離に対して急激に低下する特性を持つため、光源から離れた距離に記録層が存在する場合は、記録層に照射される光強度が低くなり、記録層を実用上十分に加熱することができないという課題が生じている。また、光源に記録層を近づけて磁気スペーシングを小さくした場合にはヘッドの浮上特性が安定しない。さらに、室温で大きな垂直磁気異方性エネルギーや保磁力を有する記録層は、キュリー温度が高く、記録温度まで多数回のエネルギー照射を行うと、保護層、記録層等に不可逆的な劣化が生じるため、多数回の記録が困難である。キュリー温度が低い記録層では、垂直磁気異方性エネルギーや保磁力が小さすぎるという課題がある。 On the other hand, the energy assist method using near-field light has a characteristic that the intensity of the near-field light rapidly decreases with respect to the distance from the light source, so when the recording layer exists at a distance away from the light source, The intensity of light applied to the recording layer is reduced, and there is a problem that the recording layer cannot be heated practically. Further, when the magnetic spacing is reduced by bringing the recording layer close to the light source, the flying characteristics of the head are not stable. Furthermore, a recording layer having a large perpendicular magnetic anisotropy energy and coercive force at room temperature has a high Curie temperature, and irreversible deterioration occurs in the protective layer, the recording layer, etc. when the energy is irradiated many times up to the recording temperature. Therefore, it is difficult to record many times. The recording layer having a low Curie temperature has a problem that the perpendicular magnetic anisotropy energy and the coercive force are too small.
 このように、大きな垂直磁気異方性エネルギーや保磁力を有し、キュリー温度が低く、磁気スペーシングが小さくても浮上特性が良い、近接場光を用いたエネルギーアシストによる磁気記録が行なえる垂直磁気記録媒体を得ることは困難であった。 In this way, it has a large perpendicular magnetic anisotropy energy and coercive force, a low Curie temperature, good flying characteristics even with a small magnetic spacing, and perpendicular recording that can perform energy-assisted magnetic recording using near-field light. It was difficult to obtain a magnetic recording medium.
 前述したように、高密度のエネルギーアシスト型垂直磁気記録を実現するには、次に述べるような種々の課題を網羅的に克服する必要がある。第1に、近接場光を用いたエネルギーアシスト用に記録層を実用上十分に加熱することができない。第2に、室温で大きな垂直磁気異方性エネルギーや高い保磁力を有し、かつキュリー温度が低い媒体を得ることが困難である。第3に、磁気スペーシングが小さい場合に、浮上特性が良い媒体を得ることが困難である。 As described above, in order to realize high-density energy-assisted perpendicular magnetic recording, it is necessary to comprehensively overcome various problems as described below. First, the recording layer cannot be heated practically enough for energy assist using near-field light. Second, it is difficult to obtain a medium having a large perpendicular magnetic anisotropy energy and a high coercive force at room temperature and a low Curie temperature. Third, it is difficult to obtain a medium having good flying characteristics when the magnetic spacing is small.
 本発明は、上述した問題点を解決して、高密度のエネルギーアシスト型垂直磁気記録を実現する垂直磁気記録媒体及び磁気記憶装置を提供することを目的とする。 An object of the present invention is to provide a perpendicular magnetic recording medium and a magnetic storage device that can solve the above-described problems and realize high-density energy-assisted perpendicular magnetic recording.
 上述課題を解決するための手段として、以下の手段を用いた。 The following means were used as means for solving the above problems.
(1)基板と、基板上に設けられた下地層及び中間層と、室温で垂直磁気異方性を有する磁気記録層と保護層を有し、エネルギー照射(アシスト)により磁気記録層の垂直磁気異方性を低下させた状態で記録を行う垂直磁気記録媒体であって、中間層がRu及び/又はPdからなり、磁気記録層は、Coを主成分とする強磁性金属層とPdを主成分とする非磁性金属層との積層体であり、強磁性金属層の膜厚が0.15以上0.25nm以下であり、非磁性金属層の膜厚が0.45以上0.8nm以下であり、強磁性金属層と非磁性金属層の膜厚比が2以上4以下であり、エネルギー照射時と非照射時の保磁力の差が8kOe以上あることを特徴とした。 (1) It has a substrate, an underlayer and an intermediate layer provided on the substrate, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature, and a protective layer, and the perpendicular magnetization of the magnetic recording layer by energy irradiation (assist) A perpendicular magnetic recording medium that performs recording in a state where anisotropy is reduced, wherein an intermediate layer is made of Ru and / or Pd, and the magnetic recording layer is mainly composed of a ferromagnetic metal layer mainly composed of Co and Pd. It is a laminate with a nonmagnetic metal layer as a component, the film thickness of the ferromagnetic metal layer is 0.15 or more and 0.25 nm or less, and the film thickness of the nonmagnetic metal layer is 0.45 or more and 0.8 nm or less. The film thickness ratio between the ferromagnetic metal layer and the nonmagnetic metal layer is 2 or more and 4 or less, and the difference in coercive force between energy irradiation and non-irradiation is 8 kOe or more.
 これにより、エネルギー照射(アシスト)により高密度の垂直磁気記録が可能となる。 This enables high-density perpendicular magnetic recording by energy irradiation (assist).
(2)基板と、基板上に設けられた下地層及び中間層と、室温で垂直磁気異方性を有する磁気記録層とキャップ層と保護層を有し、エネルギー照射により磁気記録層の垂直磁気異方性を低下させた状態で記録を行う垂直磁気記録媒体であって、中間層がRu及び/又はPduからなり、磁気記録層は、Coを主成分とする強磁性金属層とPdを主成分とする非磁性金属層との積層体であり、キャップ層がCoを主成分とする強磁性金属層とPdを主成分とする非磁性金属層との積層体からなり、強磁性金属層が0.15以上0.25nm以下であり、非磁性金属層が0.45以上0.8nm以下であり、強磁性金属層と非磁性金属層の膜厚比が2以上4以下であり、エネルギー照射時と非照射時の保磁力の差が8kOe以上あることを特徴とした。 (2) A substrate, an underlayer and an intermediate layer provided on the substrate, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature, a cap layer, and a protective layer. A perpendicular magnetic recording medium which performs recording in a state where the anisotropy is reduced, wherein the intermediate layer is made of Ru and / or Pdu, and the magnetic recording layer is mainly composed of a ferromagnetic metal layer mainly composed of Co and Pd. A non-magnetic metal layer as a component, and the cap layer is composed of a ferromagnetic metal layer mainly composed of Co and a non-magnetic metal layer mainly composed of Pd. Energy is 0.15 or more and 0.25 nm or less, the nonmagnetic metal layer is 0.45 or more and 0.8 nm or less, and the film thickness ratio of the ferromagnetic metal layer and the nonmagnetic metal layer is 2 or more and 4 or less. The difference in coercive force between time and non-irradiation is 8 kOe or more It was.
 これにより、(1)に記載の垂直磁気記録媒体の浮上特性をさらに良好にすることが可能となる。 This makes it possible to further improve the flying characteristics of the perpendicular magnetic recording medium described in (1).
(3)前記(1)又は(2)に記載の垂直磁気記録媒体において、磁気記録層のキュリー温度が220℃以上400℃以下であることを特徴とした。 (3) In the perpendicular magnetic recording medium according to (1) or (2), the Curie temperature of the magnetic recording layer is 220 ° C. or higher and 400 ° C. or lower.
 これにより、(1)又は(2)に記載の垂直磁気記録媒体の浮上特性をさらに良好にすることが可能となる。 Thereby, the flying characteristics of the perpendicular magnetic recording medium described in (1) or (2) can be further improved.
(4)前記(1)又は(2)に記載の垂直磁気記録媒体において、磁気記録層中の平均酸素濃度が5原子%以上15原子%以下であることを特徴とした。 (4) The perpendicular magnetic recording medium according to (1) or (2) is characterized in that the average oxygen concentration in the magnetic recording layer is 5 atomic% or more and 15 atomic% or less.
 これにより、面内方向の磁気相互作用を小さくし、記録ノイズを低くすることが可能となる。 This makes it possible to reduce the magnetic interaction in the in-plane direction and to reduce the recording noise.
(5)前記(1)又は(2)に記載の垂直磁気記録媒体において、強磁性金属層中の平均硼素濃度が5原子%以上15原子%以下であることを特徴とした。 (5) The perpendicular magnetic recording medium according to (1) or (2) is characterized in that the average boron concentration in the ferromagnetic metal layer is 5 atomic% or more and 15 atomic% or less.
 これにより、面内方向の粒径を小さくし、再生ノイズを低くすることが可能となる。 This makes it possible to reduce the grain size in the in-plane direction and to reduce the reproduction noise.
(6)前記(1)又は(2)に記載の垂直磁気記録媒体において、磁気記録層の膜厚が6nm以上15nm以下であることを特徴とした。 (6) In the perpendicular magnetic recording medium according to (1) or (2), the thickness of the magnetic recording layer is 6 nm or more and 15 nm or less.
 これにより、前記磁気記録層の記録時の膜厚方向の温度分布を小さくし、安定なドメインを記録することが可能となる。 This makes it possible to reduce the temperature distribution in the film thickness direction during recording of the magnetic recording layer and to record a stable domain.
(7)前記(2)に記載の垂直磁気記録媒体において、キャップ層中の平均酸素濃度が磁気記録層の平均酸素濃度より低いことを特徴とした。 (7) The perpendicular magnetic recording medium according to (2) is characterized in that the average oxygen concentration in the cap layer is lower than the average oxygen concentration in the magnetic recording layer.
 これにより、潤滑層の平坦性が向上し、浮上特性が良好な媒体を得ることが可能となる。 This improves the flatness of the lubricating layer and makes it possible to obtain a medium with good flying characteristics.
(8)前記(2)に記載の垂直磁気記録媒体において、キャップ層の膜厚が1nm以上4nm以下であることを特徴とした。 (8) In the perpendicular magnetic recording medium according to (2), the cap layer has a thickness of 1 nm to 4 nm.
 これにより、浮上特性と磁気特性の両方が良好な媒体を得ることが可能となる。 This makes it possible to obtain a medium having both good flying characteristics and magnetic characteristics.
(9)前記(1)又は(2)に記載の中間層がPdからなることを特徴とした。 (9) The intermediate layer according to (1) or (2) is characterized by being made of Pd.
 これにより、製膜時間が短縮され、生産性が向上した。 This shortened the film formation time and improved productivity.
(10)前記(1)又は(2)に記載の中間層がRuからなることを特徴とした。 (10) The intermediate layer according to (1) or (2) is characterized by being made of Ru.
 これにより、表面のラフネスが小さくなり、浮上特性が向上した。 This reduces surface roughness and improves flying characteristics.
(11)前記(1)又は(2)に記載の中間層がRuとPdからなることを特徴とした。 (11) The intermediate layer described in (1) or (2) is characterized by being made of Ru and Pd.
 これにより、生産性と浮上特性が少しずつ向上した。 This improved productivity and levitation characteristics little by little.
(12)基板と、基板上に設けられた下地層及び中間層と、室温で垂直磁気異方性を有する磁気記録層と保護層を有し、エネルギー照射により前記磁気記録層の垂直磁気異方性を低下させた状態で記録を行う垂直磁気記録媒体と、近接場光を用いたエネルギー照射機能を有する磁気記録用ヘッドと信号再生用ヘッドとを有する磁気ヘッドと備えた磁気記憶装置であって、垂直磁気記録媒体は、中間層がRu及び/又はPdからなり、磁気記録層は、Coを主成分とする強磁性金属層とPdを主成分とする非磁性金属層との積層体であり、強磁性金属層の膜厚が0.15nm以上0.25nm以下であり、非磁性金属層の膜厚が0.45nm以上0.8nm以下であり、強磁性金属層と非磁性金属層の膜厚比が2以上4以下であり、エネルギー照射時と非照射時の保磁力の差が8kOe以上あり、記録時に磁気ヘッドのエネルギー照射源から垂直磁気記録媒体の磁気記録層表面までの距離が8nm以下であることを特徴とした。 (12) A substrate, an underlayer and an intermediate layer provided on the substrate, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature, and a protective layer, and perpendicular magnetic anisotropy of the magnetic recording layer by energy irradiation A magnetic storage device comprising: a perpendicular magnetic recording medium for recording in a state of reduced performance; a magnetic recording head having an energy irradiation function using near-field light; and a magnetic head having a signal reproducing head. In the perpendicular magnetic recording medium, the intermediate layer is made of Ru and / or Pd, and the magnetic recording layer is a laminate of a ferromagnetic metal layer mainly containing Co and a nonmagnetic metal layer mainly containing Pd. The film thickness of the ferromagnetic metal layer is 0.15 nm or more and 0.25 nm or less, the film thickness of the nonmagnetic metal layer is 0.45 nm or more and 0.8 nm or less, and the film of the ferromagnetic metal layer and the nonmagnetic metal layer The thickness ratio is 2 or more and 4 or less, and energy The difference in coercivity at and during non-irradiation morphism There are more than 8 kOe, the distance from the energy radiation source of the magnetic head during recording to the magnetic recording layer surface of the perpendicular magnetic recording medium is characterized in that it is 8nm or less.
 これにより、高密度の磁気記憶装置が得られる。 As a result, a high-density magnetic storage device can be obtained.
 本発明によれば、高密度の熱アシスト記録に適した、熱アシストによる昇温で記録が可能、かつ室温では高保磁力を有する垂直磁気記録媒体及び磁気記憶装置が得られる。 According to the present invention, it is possible to obtain a perpendicular magnetic recording medium and a magnetic storage device suitable for high-density heat-assisted recording, capable of recording at a temperature rise by heat assist, and having a high coercive force at room temperature.
本発明の垂直磁気記録媒体の全体層構成を示す断面模式図。1 is a schematic cross-sectional view showing the overall layer configuration of a perpendicular magnetic recording medium of the present invention. 記録層の拡大断面図。The expanded sectional view of a recording layer. 本発明の垂直磁気記録媒体の中間層及び記録層の詳細断面構造を示す図であり、中間層まで積層された状態を示す図。FIG. 3 is a diagram showing a detailed cross-sectional structure of an intermediate layer and a recording layer of a perpendicular magnetic recording medium according to the present invention, and shows a state in which the intermediate layer is laminated. 本発明の垂直磁気記録媒体の中間層及び記録層の詳細断面構造を示す図であり、中間層上に記録層が積層された状態を示す図。FIG. 3 is a diagram showing a detailed cross-sectional structure of the intermediate layer and the recording layer of the perpendicular magnetic recording medium of the present invention, and shows a state in which the recording layer is laminated on the intermediate layer. 記録層の拡大断面図。The expanded sectional view of a recording layer. 本発明の垂直磁気記録媒体における、強磁性金属層膜厚と浮上特性、磁気特性の関係を示す図。The figure which shows the relationship between the ferromagnetic metal layer film thickness, a floating characteristic, and a magnetic characteristic in the perpendicular magnetic recording medium of this invention. 本発明の垂直磁気記録媒体における、非磁性金属層膜厚と温度特性、磁気特性の関係を示す図。The figure which shows the relationship between the film thickness of a nonmagnetic metal layer, a temperature characteristic, and a magnetic characteristic in the perpendicular magnetic recording medium of this invention. 本発明の垂直磁気記録媒体における、非磁性金属層と強磁性金属層の膜厚比と磁気特性の関係を示す図。The figure which shows the relationship between the film thickness ratio of a nonmagnetic metal layer and a ferromagnetic metal layer, and a magnetic characteristic in the perpendicular magnetic recording medium of this invention. 本発明の垂直磁気記録媒体の保磁力差と信号劣化量の関係を示す図。The figure which shows the relationship between the coercive force difference of the perpendicular magnetic recording medium of this invention, and signal degradation amount. 本発明の垂直磁気記録媒体における、記録層中の酸素量と結晶化特性の関係を示す図。The figure which shows the relationship between the amount of oxygen in a recording layer, and the crystallization characteristic in the perpendicular magnetic recording medium of this invention. 本発明の垂直磁気記録媒体における、強磁性金属層中の硼素量と磁気特性、結晶粒径の関係を示す図。The figure which shows the relationship between the amount of boron in a ferromagnetic metal layer, a magnetic characteristic, and a crystal grain diameter in the perpendicular magnetic recording medium of this invention. 本発明のキャップ層を有する垂直磁気記録媒体の全体層構成を示す断面模式図。FIG. 2 is a schematic cross-sectional view showing the entire layer structure of a perpendicular magnetic recording medium having a cap layer of the present invention. キャップ層の拡大図。The enlarged view of a cap layer. 本発明のキャップ層を有する垂直磁気記録媒体の詳細断面構造を示す図。The figure which shows the detailed cross-section of the perpendicular magnetic recording medium which has a cap layer of this invention. 記録層の拡大断面図。The expanded sectional view of a recording layer. 本発明のキャップ層を有する垂直磁気記録媒体と比較例の媒体における磁気特性を示す図。The figure which shows the magnetic characteristic in the perpendicular magnetic recording medium which has a cap layer of this invention, and the medium of a comparative example. 本発明の磁気記憶装置の構成例を示す平面模式図。1 is a schematic plan view showing a configuration example of a magnetic storage device of the present invention. 図12AのA-A’断面図。FIG. 12A is a cross-sectional view taken along the line A-A ′ of FIG. 12A. 本発明の磁気記憶装置に搭載されたヘッドの概略図。1 is a schematic view of a head mounted on a magnetic storage device of the present invention. ヘッド主要部の側面から見た概略図。Schematic view seen from the side of the main part of the head. 本発明の磁気記憶装置における、エネルギー源から記録層表面までの距離と吸収率の関係を示す図。The figure which shows the relationship between the distance from an energy source to the surface of a recording layer, and an absorptance in the magnetic memory device of this invention.
 以下、図面を参照して本発明の実施の形態を説明する。 Hereinafter, embodiments of the present invention will be described with reference to the drawings.
[実施例1]
 本発明の一つの実施例として、室温で垂直磁気異方性を有する磁気記録層を有し、エネルギー照射(アシスト)により垂直磁気異方性を低下させた状態で記録を行う垂直磁気記録媒体を説明する。ここでは、近接場光を用いてエネルギーアシストを行った。これにより、媒体中の加熱される領域の直径が数+nm以下と非常に狭い範囲に局所的にエネルギー照射出来る。エネルギーの照射量は、媒体の温度がキュリー点の約70%以上になるように最適化して評価を行った。
[Example 1]
As one embodiment of the present invention, a perpendicular magnetic recording medium having a magnetic recording layer having perpendicular magnetic anisotropy at room temperature and performing recording in a state where the perpendicular magnetic anisotropy is reduced by energy irradiation (assist) is provided. explain. Here, energy assist was performed using near-field light. As a result, energy can be locally irradiated in a very narrow range in which the diameter of the heated region in the medium is several + nm or less. The energy dose was optimized and evaluated so that the temperature of the medium was about 70% or more of the Curie point.
 図1(a)は、本発明の一つの実施例として強磁性金属層108と非磁性金属層109の多層膜からなる記録層104を有する垂直磁気記録媒体の断面構造を模式的に示したものである。基板101上に、下地層102として約30nmのNi63Ta38層と約7nmのNi946層、中間層103として約16nmのRu層、約12nmの記録層104、保護層106として約3nmのCN層を順次形成した。製膜は、それぞれDCスパッタリングにて行った。その後、CN層の上に、約1nmの潤滑材107を塗布した。図1(b)は、記録層104を拡大した概念図である。記録層104には、強磁性金属層108にはCo9010、非磁性金属層109にはPdを用いた。多層膜の形成は、基板を固定し、回転型のカソードを用い、Co9010のターゲットとPdターゲットを回転させながら、両層を交互に形成し、合計約12nm製膜した。図1(b)では簡略化されているが、記録層104中は、各構成層として強磁性金属層108を0.2nm、非磁性金属層109を0.6nm、交互に15回積層されている。多層膜の場合の垂直磁気異方性の起源は、主に界面であるため、両者の層が交互に積層されて界面が形成されることが重要であり、強磁性金属層と非磁性金属層のどちらが先に製膜されていてもよい。ターゲットを固定し、基板を回転させても同様の多層膜が形成できる。各構成層の膜厚は、各ターゲットに投入するパワーを変えることにより、変化させた。また、多層記録層に粒界構造を形成するため、製膜時に微量の酸素を添加した。 FIG. 1A schematically shows a cross-sectional structure of a perpendicular magnetic recording medium having a recording layer 104 composed of a multilayer film of a ferromagnetic metal layer 108 and a nonmagnetic metal layer 109 as one embodiment of the present invention. It is. On the substrate 101, a Ni 63 Ta 38 layer of about 30 nm and a Ni 94 W 6 layer of about 7 nm as the underlayer 102, a Ru layer of about 16 nm as the intermediate layer 103, a recording layer 104 of about 12 nm, and a protective layer 106 of about 3 nm CN layers were sequentially formed. Film formation was performed by DC sputtering. Thereafter, about 107 nm of the lubricant 107 was applied on the CN layer. FIG. 1B is an enlarged conceptual diagram of the recording layer 104. For the recording layer 104, Co 90 B 10 was used for the ferromagnetic metal layer 108, and Pd was used for the nonmagnetic metal layer 109. The multilayer film was formed by alternately forming both layers while fixing the substrate and rotating the Co 90 B 10 target and the Pd target using a rotating cathode, and formed a total film of about 12 nm. Although simplified in FIG. 1B, in the recording layer 104, the ferromagnetic metal layer 108 and the nonmagnetic metal layer 109 are alternately laminated 15 times as the constituent layers by 0.2 nm and 0.6 nm, respectively. Yes. Since the origin of perpendicular magnetic anisotropy in the case of a multilayer film is mainly the interface, it is important that the two layers are alternately stacked to form an interface, and a ferromagnetic metal layer and a nonmagnetic metal layer Either of these may be formed first. A similar multilayer film can be formed by fixing the target and rotating the substrate. The film thickness of each constituent layer was changed by changing the power input to each target. Further, in order to form a grain boundary structure in the multilayer recording layer, a small amount of oxygen was added during film formation.
 中間層103は、図2に示すように、低ガス圧(1.4Pa)で第1中間層201としてRuを8nm形成した後、高ガス圧(5Pa)で第2中間層202としてRuを8nm形成した。このように、低ガス圧で平坦な膜を製膜して結晶性を整え、その上に高ガス圧で製膜して凹凸形状を形成(図2(a))することにより、お椀型の粒が分離した形状の上に垂直方向に結晶配向性の良い多層記録層104が形成できる(図2(b))。強磁性金属層108と非磁性金属層109の多層膜は主に結晶粒203中に形成されている(図2(c))。中間層製膜時のガス圧の範囲としては、低ガス圧は1~2Pa、高ガス圧は4~10Paにした場合、凹凸形状を形成し、記録層の分離促進と結晶配向性を良好にする効果が得られた。 As shown in FIG. 2, the intermediate layer 103 is formed with 8 nm of Ru as the first intermediate layer 201 at a low gas pressure (1.4 Pa), and then 8 nm of Ru as the second intermediate layer 202 at a high gas pressure (5 Pa). Formed. In this way, a flat film is formed at a low gas pressure to adjust the crystallinity, and a film is formed thereon at a high gas pressure to form a concavo-convex shape (FIG. 2A). A multilayer recording layer 104 having good crystal orientation in the vertical direction can be formed on the shape in which the grains are separated (FIG. 2B). The multilayer film of the ferromagnetic metal layer 108 and the nonmagnetic metal layer 109 is mainly formed in the crystal grains 203 (FIG. 2C). As the range of gas pressure during intermediate layer deposition, when the low gas pressure is 1 to 2 Pa and the high gas pressure is 4 to 10 Pa, the uneven shape is formed, and the separation of the recording layer is promoted and the crystal orientation is improved. The effect to do was obtained.
 まず、記録層について調べた。非磁性金属層の膜厚を0.6nmと一定にし、強磁性金属層の浮上特性と飽和磁化の膜厚依存性を調べた。その結果を、図3及び表1に示す。 First, the recording layer was examined. The thickness of the nonmagnetic metal layer was kept constant at 0.6 nm, and the floating characteristics of the ferromagnetic metal layer and the thickness dependence of the saturation magnetization were investigated. The results are shown in FIG.

               表1
強磁性金属層の膜厚(nm) 浮上特性(mV)  飽和磁化(emu/cc)
   0.05         31.3        -
   0.1          31.3       212
   0.15         31.3       301
   0.17         31.3       320
   0.2          31.3       336
   0.23         31.4       359
   0.25         31.5        -
   0.3          31.8       403
   0.4          32.7       413

Table 1
Ferromagnetic metal layer thickness (nm) Flying characteristics (mV) Saturation magnetization (emu / cc)
0.05 31.3-
0.1 31.3 212
0.15 31.3 301
0.17 31.3 320
0.2 31.3 336
0.23 31.4 359
0.25 31.5-
0.3 31.8 403
0.4 32.7 413
 この場合、構成層の積層数は18から12回となるが、磁気モーメントは記録層膜厚に比例するため、記録層の総膜厚を約12nmと一定として比較を行った。浮上特性は、専用のピエゾ電気センサー端子をヘッドに取り付けた磁気ヘッドを有するテスタにて、ヘッド浮上時のピエゾ端子振動の出力をプロットして測定した。媒体の潤滑材表面が平坦でヘッドが媒体に衝突することなく安定に浮上しているほど、振動は少ないため、出力は小さくなる。安定に浮上している場合、ピエゾ出力は31.5mV以下となり、掠ったり、衝突したりするなど浮上が不安定になるほど振動が大きくなるため、出力は大きくなる。実用的に媒体が使用されるためには、ヘッドの衝突等が生じてはならないため、ピエゾ出力は31.5mV以下であることが重要である。さらに、31.4mV以下は、外部振動などの外乱が生じても、媒体とヘッドとが衝突しないレベルであり、より好ましい。飽和磁化は、媒体を小片に切断した後、振動磁気磁針計(VSM)を用いて測定を行った。本明細書中で特に温度の記載がない評価に関しては全て室温で行った。飽和磁化が小さいと、ビットが記録された際の信号レベルが低くなり、SNRが低くなってしまい正しく記録された情報を再生することが出来ない。このため、飽和磁化が290emu/cc以上であることが重要となる。 In this case, the number of constituent layers is 18 to 12, but since the magnetic moment is proportional to the recording layer thickness, the total thickness of the recording layer was constant at about 12 nm. The flying characteristics were measured by plotting the output of the piezoelectric terminal vibration when the head floated with a tester having a magnetic head with a dedicated piezoelectric sensor terminal attached to the head. The flatter the lubricant surface of the medium and the more stable the head flies without colliding with the medium, the smaller the output, and the smaller the output. When the levitation is stable, the piezo output is 31.5 mV or less, and the vibration becomes larger as the levitation becomes unstable, such as hitting or colliding, and the output increases. In order for the medium to be used practically, a head collision or the like should not occur, so it is important that the piezo output is 31.5 mV or less. Furthermore, 31.4 mV or less is more preferable because it is a level at which the medium and the head do not collide even when a disturbance such as external vibration occurs. The saturation magnetization was measured using a vibrating magnetic magnetometer (VSM) after the medium was cut into small pieces. In the present specification, evaluations not particularly described in temperature were all performed at room temperature. If the saturation magnetization is small, the signal level when the bit is recorded becomes low, the SNR becomes low, and the correctly recorded information cannot be reproduced. For this reason, it is important that the saturation magnetization is 290 emu / cc or more.
 図3及び表1より、強磁性金属層の膜厚が薄いほどヘッド浮上時のピエゾ出力が小さく浮上特性が良好になり、厚いほど飽和磁化が大きくなることがわかる。強磁性金属層の膜厚が0.15nm以上0.25nm以下の場合に、ピエゾ出力が31.5mV以下、飽和磁化が290emu/cc以上と、浮上特性及び磁気特性の両者が良好な結果が得られた。さらに、強磁性金属層の膜厚が0.17nm以上0.23nm以下の場合に、ピエゾ出力が31.4mV以下、飽和磁化が310emu/cc以上と、浮上特性及び磁気特性の両者がより良好な結果が得られた。 3 and Table 1, it can be seen that the thinner the ferromagnetic metal layer, the smaller the piezo output at the time of flying the head, and the better the flying characteristics, and the thicker the saturation magnetization becomes. When the thickness of the ferromagnetic metal layer is 0.15 nm or more and 0.25 nm or less, the piezoelectric output is 31.5 mV or less and the saturation magnetization is 290 emu / cc or more. It was. Furthermore, when the thickness of the ferromagnetic metal layer is 0.17 nm or more and 0.23 nm or less, the piezo output is 31.4 mV or less, the saturation magnetization is 310 emu / cc or more, and both the floating characteristics and the magnetic characteristics are better. Results were obtained.
 強磁性金属層の膜厚を0.2nmと一定にし、温度特性と飽和磁化の、非磁性金属層の膜厚依存性を調べた。結果を図4及び表2に示す。 The film thickness of the ferromagnetic metal layer was kept constant at 0.2 nm, and the dependence of the temperature characteristics and saturation magnetization on the film thickness of the nonmagnetic metal layer was investigated. The results are shown in FIG.

               表2
非磁性金属層の膜厚(nm)  飽和磁化(emu/cc) キュリー温度(℃)
   1.0           210      150
   0.8           296      220
   0.7           310      280
   0.6           336      320
   0.5           ―        370
   0.45          385      400
   0.4           405      420
   0.3           425       -

Table 2
Nonmagnetic metal layer thickness (nm) Saturation magnetization (emu / cc) Curie temperature (° C)
1.0 210 150
0.8 296 220
0.7 310 280
0.6 336 320
0.5-370
0.45 385 400
0.4 405 420
0.3 425-
 この場合、構成層の積層数は10から24回となるが、磁気モーメントは記録層膜厚に比例するため、記録層の総膜厚を約12nmと一定として比較を行った。温度特性は、媒体を小片に切断した後、ヒーターにて加熱を行いながら、各温度における飽和磁化を測定して求め、飽和磁化が20emu/cc以下と十分小さくなった温度をキュリー温度とした。エネルギー照射により、垂直磁気異方性を低下させて記録を行う方式では、温度特性も重要な物性の一つである。キュリー温度が低すぎる場合は、少量のエネルギー照射で飽和磁化が低下してしまうため、エネルギー照射量の制御が困難となる。そこで、室温から十分離れた温度にする必要があり、キュリー温度220℃以上が好ましい。一方で、キュリー温度が高い場合、記録のために記録層をより高温にする必要があるが、記録層が400℃以上になると、保護層や潤滑材の熱劣化が生じてしまう。保護層等が劣化すると、記録層が大気に曝され磁気特性が劣化したり、保護層や潤滑材表面に凹凸が生じ浮上特性が劣化したりする。そのため、キュリー温度は400℃以下が好ましい。 In this case, the number of constituent layers is 10 to 24, but since the magnetic moment is proportional to the thickness of the recording layer, the total thickness of the recording layer was kept constant at about 12 nm. The temperature characteristics were obtained by measuring the saturation magnetization at each temperature while heating with a heater after cutting the medium into small pieces, and the temperature at which the saturation magnetization was sufficiently small at 20 emu / cc or less was taken as the Curie temperature. In the method of recording by reducing the perpendicular magnetic anisotropy by energy irradiation, the temperature characteristic is also an important physical property. When the Curie temperature is too low, the saturation magnetization is lowered by a small amount of energy irradiation, so that it is difficult to control the energy irradiation amount. Therefore, it is necessary to set the temperature sufficiently away from room temperature, and a Curie temperature of 220 ° C. or higher is preferable. On the other hand, when the Curie temperature is high, it is necessary to make the recording layer higher for recording. However, when the recording layer reaches 400 ° C. or more, the protective layer and the lubricant are thermally deteriorated. When the protective layer or the like deteriorates, the recording layer is exposed to the atmosphere and the magnetic characteristics deteriorate, or the surface of the protective layer or the lubricant material becomes uneven and the flying characteristics deteriorate. Therefore, the Curie temperature is preferably 400 ° C. or lower.
 図4及び表2より、非磁性金属層の膜厚が薄いほど飽和磁化が大きくなり、厚いほどキュリー温度が低くなることがわかる。非磁性金属層の膜厚が0.45nm以上0.8nm以下の場合に、キュリー温度が400℃以下、飽和磁化が290emu/cc以上と、温度特性及び磁気特性の両者が良好な結果が得られた。さらに、非磁性金属層の膜厚が0.5nm以上0.7nm以下の場合に、キュリー温度が370℃以下、飽和磁化が310emu/cc以上と、温度特性及び磁気特性の両者がより良好な結果が得られた。 4 and Table 2, it can be seen that the saturation magnetization increases as the film thickness of the nonmagnetic metal layer decreases, and the Curie temperature decreases as the film thickness increases. When the film thickness of the nonmagnetic metal layer is 0.45 nm or more and 0.8 nm or less, the Curie temperature is 400 ° C. or less and the saturation magnetization is 290 emu / cc or more. It was. Furthermore, when the film thickness of the nonmagnetic metal layer is 0.5 nm or more and 0.7 nm or less, the Curie temperature is 370 ° C. or less, the saturation magnetization is 310 emu / cc or more, and both the temperature characteristics and the magnetic characteristics are better. was gotten.
 図5及び表3に、非磁性金属層と強磁性金属層の膜厚比をかえながら、磁気特性を調べた結果を示す。 FIG. 5 and Table 3 show the results of examining the magnetic characteristics while changing the film thickness ratio between the nonmagnetic metal layer and the ferromagnetic metal layer.
                表3
 強磁性金属層の膜厚  非磁性金属層の膜厚  膜厚比   保磁力
   (nm)       (nm)           (kOe)
   0.9        0.15      6     7.1
   0.75       0.15      5     8.0
   0.8        0.2       4     9.1
   0.7        0.2       3.5  10.5
   0.6        0.2       3    11.7
   0.5        0.2       2.5  10.5
   0.5        0.25      2     9.4
   0.45       0.3       1.5   7.2
Table 3
Film thickness of ferromagnetic metal layer Film thickness of nonmagnetic metal layer Film thickness ratio Coercive force (nm) (nm) (kOe)
0.9 0.15 6 7.1
0.75 0.15 5 8.0
0.8 0.2 4 9.1
0.7 0.2 3.5 10.5
0.6 0.2 3 11.7
0.5 0.2 2.5 10.5
0.5 0.25 2 9.4
0.45 0.3 1.5 7.2
 ここでは、カー効果測定装置を用い、保磁力を調べた。保磁力が低いと記録された領域のうち不安定な領域が、ヘッド磁界やヘッド周辺温度上昇等により消滅してしまうため、室温における保磁力はヘッド磁界約6kOeから50%以上大きい9kOe以上が好ましい。図5及び表3より、非磁性金属層と強磁性金属層の膜厚比が適当な範囲で保磁力が大きくなることがわかる。非磁性金属層と強磁性金属層の膜厚比が2以上4以下の場合に、保磁力9kOe以上と良好な結果が得られた。さらに、非磁性金属層と強磁性金属層の膜厚比が2.5以上3.5以下の場合に、保磁力10.5kOe以上とより良好な結果が得られた。 Here, the coercive force was examined using a Kerr effect measuring device. If the coercive force is low, an unstable region of the recorded region disappears due to a head magnetic field, a rise in the temperature around the head, or the like. . From FIG. 5 and Table 3, it can be seen that the coercive force increases when the film thickness ratio between the nonmagnetic metal layer and the ferromagnetic metal layer is in an appropriate range. When the film thickness ratio between the nonmagnetic metal layer and the ferromagnetic metal layer was 2 or more and 4 or less, a coercive force of 9 kOe or more was obtained. Furthermore, when the film thickness ratio between the nonmagnetic metal layer and the ferromagnetic metal layer was 2.5 or more and 3.5 or less, a better result was obtained with a coercive force of 10.5 kOe or more.
 表4には、膜厚比を一定にして、磁性金属層と強磁性金属層の膜厚が上記良好な範囲内に入っている場合と範囲外の場合を比較した結果を示す。 Table 4 shows a result of comparing the case where the film thickness ratio is constant and the film thickness of the magnetic metal layer and the ferromagnetic metal layer is within the above-mentioned preferable range and the case outside the range.

                表4
番号 強磁性金属層の膜厚 非磁性金属層の膜厚 膜厚比  保磁力
    (nm)      (nm)         (kOe)
41   0.4       1.2      3    7.1
42   0.2       0.6      3   11.7
43   0.1       0.3      3    3.5
44   0.08      0.24     3    2.7

Table 4
Number Thickness of ferromagnetic metal layer Thickness of nonmagnetic metal layer Thickness ratio Coercivity
(Nm) (nm) (kOe)
41 0.4 1.2 3 7.1
42 0.2 0.6 3 11.7
43 0.1 0.3 3 3.5
44 0.08 0.24 3 2.7
 これより、非磁性金属層と強磁性金属層の膜厚比が適当な範囲であっても、構成層の膜厚が適当な範囲から外れた際(番号41,43,44)、つまりここでは強磁性金属層の膜厚が0.4,0.1,0.08nmの場合には、保磁力が9kOeより小さい。以上をまとめると、各構成層の膜厚及び膜厚比全てが良好な範囲にある場合にのみ、浮上特性、磁気特性、温度特性の良好な結果を得ることが出来た。 Thus, even when the film thickness ratio between the nonmagnetic metal layer and the ferromagnetic metal layer is in an appropriate range, when the film thickness of the constituent layer is out of the appropriate range (numbers 41, 43, 44), that is, here When the thickness of the ferromagnetic metal layer is 0.4, 0.1, 0.08 nm, the coercive force is smaller than 9 kOe. In summary, only when the film thickness and the film thickness ratio of each constituent layer are in a good range, good results of flying characteristics, magnetic characteristics, and temperature characteristics could be obtained.
 図6及び表5に、エネルギー照射時と非照射時の保磁力差と信号劣化量の関係を調べた結果を示す。 Fig. 6 and Table 5 show the results of examining the relationship between the difference in coercive force during energy irradiation and non-irradiation and the signal degradation amount.
            表5
   保磁力    保磁力差   信号劣化量
  (kOe)   (kOe)   (dB) 
   4.7     3.7     5
   7.1     6.1     1
   9.0     8.0     0.2
  10.5     9.5     0
  11.7    10.7     0
Table 5
Coercive force Coercive force difference Signal degradation (kOe) (kOe) (dB)
4.7 3.7 5
7.1 6.1 1
9.0 8.0 0.2
10.5 9.5 0
11.7 10.7 0
 記録時のエネルギー光源波長は780nm、エネルギー光源の出射パワーは100mW、エネルギー照射時間は2ns、記録磁界は約6kOe、媒体は上記図1に記載の構造を用いた。測定は、次のような手順で行った。エネルギーアシストにより、線記録密度1500fciで記録を行った後、信号レベルを測定した。次に、両隣のトラックに線記録密度1000fciで記録を行い、最初に記録しておいた信号のレベルを再度測定した。両脇のトラックに記録する際に、既に記録したトラックも隣接トラックから洩れたヘッド磁界や温度上昇にさらされる。このため、保磁力差が低く不十分な媒体では、記録ビット領域内の一部が消滅してしまい、信号劣化が生じる。信号劣化量は、最初に記録した場合と、両脇に記録を行った場合の信号レベルの差を信号劣化量として算出した。 The energy light source wavelength during recording was 780 nm, the emission power of the energy light source was 100 mW, the energy irradiation time was 2 ns, the recording magnetic field was about 6 kOe, and the medium shown in FIG. 1 was used. The measurement was performed according to the following procedure. After recording with energy assist at a linear recording density of 1500 fci, the signal level was measured. Next, recording was performed on the adjacent tracks at a linear recording density of 1000 fci, and the level of the signal recorded first was measured again. When recording on the tracks on both sides, the already recorded track is also exposed to the head magnetic field and temperature rise leaked from the adjacent track. For this reason, in a medium having a low coercive force difference and insufficient, a part of the recording bit area disappears and signal degradation occurs. The signal degradation amount was calculated as the signal degradation amount by the difference in signal level between the first recording and the recording on both sides.
 信号劣化が1%以上生じると、エラーコレクションで劣化信号を救うことが難しくなる。また、エラーコレクションを行うには、エラーコレクション用の余分のコードを記録することが必要になるため、劣化信号が少ないほど記録密度の低下が抑制でき、信号劣化が0%だとより好ましい。図6及び表5より、保磁力差が大きいほど信号劣化が生じないことがわかる。エネルギー照射時と非照射時の保磁力差が8kOe以上の場合に、信号劣化量は0.2dB以下に抑えられ、良好な結果が得られた。さらに、エネルギー照射時と非照射時の保磁力差が9.5kOe以上の場合に、信号劣化量は0dBに抑えられ、より良好な結果が得られた。 If signal degradation occurs more than 1%, it becomes difficult to save the degradation signal by error correction. Further, since error correction requires recording extra codes for error correction, the smaller the deterioration signal, the lower the recording density can be suppressed, and the signal deterioration is more preferably 0%. From FIG. 6 and Table 5, it can be seen that signal deterioration does not occur as the coercive force difference increases. When the difference in coercive force between energy irradiation and non-irradiation was 8 kOe or more, the signal deterioration amount was suppressed to 0.2 dB or less, and good results were obtained. Furthermore, when the difference in coercive force between energy irradiation and non-irradiation was 9.5 kOe or more, the signal deterioration amount was suppressed to 0 dB, and a better result was obtained.
 次に、中間層材料依存性を調べた。強磁性金属層の膜厚を0.2nm、非磁性金属層の膜厚を0.6nm、記録層の総膜厚を12nmと一定にし、中間層材料及び製膜プロセスの組合せを変えながら、保磁力を調べた。中間層を前記のように低ガス圧と高ガス圧の製膜プロセスにて形成した場合と、単一製膜プロセスにて形成した場合についても比較を行った。表6にその結果をまとめた。 Next, the intermediate layer material dependency was examined. The ferromagnetic metal layer thickness is 0.2 nm, the non-magnetic metal layer thickness is 0.6 nm, the total recording layer thickness is 12 nm, and the combination of the intermediate layer material and the film forming process is changed. The magnetic force was examined. A comparison was also made between the case where the intermediate layer was formed by the low gas pressure and high gas pressure film forming processes and the case where the intermediate layer was formed by a single film forming process. Table 6 summarizes the results.

                 表6
番号              中間層          保磁力
                            (kOe) 
61  Pd(低ガス圧、8nm)/Pd(高ガス圧、8nm) 13.5
62  Ru(低ガス圧、8nm)/Pd(高ガス圧、8nm) 12.2
63  Ru(低ガス圧、8nm)/Ru(高ガス圧、8nm) 11.7
64  Pd(低ガス圧、8nm)/Ru(高ガス圧、8nm) 11.5
65  Pd(低ガス圧、16nm)             11.1
66  Ru(低ガス圧、16nm)             10.6
67  なし                         6.4
68  Co(低ガス圧、16nm)              4.4
69  Co(低ガス圧、8nm)/Pd(高ガス圧、8nm)  4.1

Table 6
No.
(KOe)
61 Pd (low gas pressure, 8 nm) / Pd (high gas pressure, 8 nm) 13.5
62 Ru (low gas pressure, 8 nm) / Pd (high gas pressure, 8 nm) 12.2
63 Ru (low gas pressure, 8 nm) / Ru (high gas pressure, 8 nm) 11.7
64 Pd (low gas pressure, 8 nm) / Ru (high gas pressure, 8 nm) 11.5
65 Pd (low gas pressure, 16 nm) 11.1
66 Ru (low gas pressure, 16 nm) 10.6
67 None 6.4
68 Co (low gas pressure, 16 nm) 4.4
69 Co (low gas pressure, 8 nm) / Pd (high gas pressure, 8 nm) 4.1
 このように、中間層材料がRu及び/又はPdの場合、9kOeの大きな保磁力が得られた。しかし、記録層の構成が良好な組成にもかかわらず、中間層材料がRu,Pd以外の場合、又は中間層を形成しなかった場合は、保磁力が4~6kOeと小さかった。また、中間層が単層の場合に保磁力が低めなのは、結晶粒の分離が不十分なためと考えられる。中間層材料として、Ruが良好な特性を示しているのは、hcp構造の結晶によりCo層のc軸又はPd層の(111)配向性を向上させたのに加えて凹凸形状を形成し、記録層の垂直磁気異方性を形成しやすいためと考えられる。同じhcp構造のCoは、凹凸形状の形成が少なく良好な保磁力が得られなかった。Pdは、fcc構造であるが、凹凸形状が大きく、結晶粒の分離が促進されたため、保磁力が大きくなったと考えられる。また、Pdは製膜レートが早いため、高ガス圧での製膜にPdを用いると量産性が向上できる。しかしながら、表面ラフネスは大きく、番号61のラフネスは番号63の1.5倍、番号62は番号63の1.3倍であった。 Thus, when the intermediate layer material was Ru and / or Pd, a large coercive force of 9 kOe was obtained. However, although the composition of the recording layer was good, the coercive force was as small as 4 to 6 kOe when the intermediate layer material was other than Ru and Pd, or when the intermediate layer was not formed. Moreover, when the intermediate layer is a single layer, the coercive force is low because the crystal grains are not sufficiently separated. As an intermediate layer material, Ru has good characteristics because the hcp structure crystal improves the c-axis of the Co layer or the (111) orientation of the Pd layer, and forms an uneven shape. This is probably because the perpendicular magnetic anisotropy of the recording layer is easily formed. Co having the same hcp structure has little formation of uneven shapes and a good coercive force could not be obtained. Although Pd has an fcc structure, it is considered that the coercive force is increased because the uneven shape is large and the separation of crystal grains is promoted. Further, since Pd has a high film formation rate, mass production can be improved by using Pd for film formation at a high gas pressure. However, the surface roughness was large, the roughness of number 61 was 1.5 times that of number 63, and number 62 was 1.3 times that of number 63.
 以上より、基板と、基板上に設けられた下地層及び中間層と、室温で垂直磁気異方性を有する磁気記録層と保護層を有し、エネルギー照射により垂直磁気異方性を低下させた状態で記録を行う垂直磁気記録媒体において、中間層をRu及び/又はPdから形成し、磁気記録層を、Coを主成分とする強磁性金属層とPdを主成分とする非磁性金属層との積層体とし、強磁性金属層の膜厚を0.15nm以上0.25nm以下とし、非磁性金属層の膜厚を0.45nm以上0.8nm以下とし、強磁性金属層と非磁性金属層の膜厚比を2以上4以下とし、エネルギー照射時と非照射時の保磁力の差を8kOe以上とすることにより、良好な記録再生特性を有する、エネルギーアシスト型垂直磁気記録媒体を得ることが可能となる。 As described above, it has a substrate, an underlayer and an intermediate layer provided on the substrate, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature, and a protective layer, and the perpendicular magnetic anisotropy is reduced by energy irradiation. In a perpendicular magnetic recording medium that performs recording in a state, an intermediate layer is formed of Ru and / or Pd, and the magnetic recording layer includes a ferromagnetic metal layer mainly containing Co and a nonmagnetic metal layer mainly containing Pd. The ferromagnetic metal layer has a thickness of 0.15 nm to 0.25 nm and the nonmagnetic metal layer has a thickness of 0.45 nm to 0.8 nm. By setting the film thickness ratio to 2 to 4 and the difference in coercivity between energy irradiation and non-irradiation to 8 kOe or more, an energy-assisted perpendicular magnetic recording medium having good recording / reproducing characteristics can be obtained. It becomes possible.
 この他、基板101には、直径2.5インチ、厚さ0.6mm、表面ラフネスRaが0.3nm以下の強化ガラスを用いたが、直径が3.5インチ、5インチや1.8インチ等、厚さが1mm、0.8mm、0.5mm等、別のサイズの基板を用いてもよい。基板の材質は、強化ガラス以外でも良いが、Si、アルミなど表面が500℃程度にさらされても変形・変質しない材料が好ましい。 In addition, for the substrate 101, tempered glass having a diameter of 2.5 inches, a thickness of 0.6 mm, and a surface roughness Ra of 0.3 nm or less was used, but the diameter was 3.5 inches, 5 inches, or 1.8 inches. For example, a substrate having a different size such as 1 mm, 0.8 mm, or 0.5 mm may be used. The material of the substrate may be other than tempered glass, but a material such as Si or aluminum that does not deform or change even when the surface is exposed to about 500 ° C. is preferable.
 下地層102にはNi63Ta38層とNi946層を用いたが、基板、中間層との密着性や平坦性を確保できれば、このほかの材料や膜厚でも良い。保護層106についても、記録層との密着性、熱アシスト光源の波長における透明性、表面の平坦性が確保できれば、組成比が異なっていてもよく、この他の材料でもよい。 Although the Ni 63 Ta 38 layer and the Ni 94 W 6 layer were used for the underlayer 102, other materials and film thicknesses may be used as long as adhesion and flatness with the substrate and the intermediate layer can be secured. The protective layer 106 may have a different composition ratio or other materials as long as adhesion to the recording layer, transparency at the wavelength of the heat-assisted light source, and surface flatness can be ensured.
 また、強磁性金属層の膜厚を0.2nm、非磁性金属層の膜厚を0.6nm、記録層の総膜厚を12nmとして、製膜中のArガスへの酸素添加量を変えながら製膜し、膜中の酸素量及び記録層の結晶配向及び結晶の粒界幅の関係を調べたところ、図7及び表7に示す結果が得られた。 Further, the film thickness of the ferromagnetic metal layer is 0.2 nm, the film thickness of the nonmagnetic metal layer is 0.6 nm, the total film thickness of the recording layer is 12 nm, and the amount of oxygen added to the Ar gas during film formation is changed. When the relationship between the amount of oxygen in the film, the crystal orientation of the recording layer, and the grain boundary width of the crystal was examined, the results shown in FIG. 7 and Table 7 were obtained.
             表7
番号  酸素量(原子%) 結晶配向(°) 結晶粒界幅(nm)
71    0      3.19    0
72    5      3.21    0.3
73    8      3.25    0.4
74   10      3.28    0.5
75   13      3.3     0.55
76   15      3.32    0.6
77   19      3.43    0.8
Table 7
Number Oxygen content (atomic%) Crystal orientation (°) Grain boundary width (nm)
71 0 3.19 0
72 5 3.21 0.3
73 8 3.25 0.4
74 10 3.28 0.5
75 13 3.3 0.55
76 15 3.32 0.6
77 19 3.43 0.8
 酸素量の分析は、エネルギー分散型X線分析装置(EDX)にて行った。結晶配向性は、X線回折装置を用いて調べた。結晶配向性が良いほど、結晶ごとの磁気特性が均一になる。結晶配向性が劣化すると、磁気特性の分散が大きくなり、ノイズの原因となるため、結晶配向は3.35゜以下が好ましい。結晶粒界幅は、透過型電子顕微鏡(TEM)により、100個の粒子の粒及び粒界の観察を行い、粒界の平均値を求めた。結晶粒界幅が大きいほど、隣接粒子の磁気的な影響を受けなくなる。つまり、磁気的な相関距離が小さくなり、記録エラー率が減少する。そのため、結晶粒界は大きいことが必要で、少なくとも0.3nm以上が好ましい。結晶粒界が形成されない場合、磁気的な相関距離が大きすぎ、ビット長25nmといった、高密度のビットは形成できない。 The oxygen amount was analyzed using an energy dispersive X-ray analyzer (EDX). The crystal orientation was examined using an X-ray diffractometer. The better the crystal orientation, the more uniform the magnetic properties of each crystal. When the crystal orientation deteriorates, the dispersion of magnetic characteristics increases and causes noise. Therefore, the crystal orientation is preferably 3.35 ° or less. The grain boundary width was determined by observing 100 grains and grain boundaries with a transmission electron microscope (TEM), and obtaining an average value of the grain boundaries. The larger the grain boundary width, the less magnetic influence of adjacent particles. That is, the magnetic correlation distance is reduced and the recording error rate is reduced. Therefore, the crystal grain boundary needs to be large, and is preferably at least 0.3 nm or more. When the grain boundary is not formed, the magnetic correlation distance is too large, and a high-density bit such as a bit length of 25 nm cannot be formed.
 図7及び表7より、酸素量が増加するほど、結晶配向性は悪化し、結晶粒界幅は大きくなることがわかる。記録層中の酸素量が5原子%以上15原子%以下の場合に、結晶配向は3.35°以下、結晶粒界幅は0.3nm以上に出来、良好な結果が得られた。さらに、記録層中の酸素量が8原子%以上13原子%以下の場合に、結晶配向は3.3°以下、結晶粒界幅は0.4nm以上に出来、より良好な結果が得られた。 7 and Table 7 that the crystal orientation deteriorates and the grain boundary width increases as the amount of oxygen increases. When the amount of oxygen in the recording layer was 5 atom% or more and 15 atom% or less, the crystal orientation was 3.35 ° or less and the grain boundary width was 0.3 nm or more, and good results were obtained. Further, when the oxygen content in the recording layer is 8 atomic% or more and 13 atomic% or less, the crystal orientation can be 3.3 ° or less and the grain boundary width can be 0.4 nm or more, and a better result is obtained. .
 さらに、強磁性金属層中へB(硼素)を添加することで、結晶粒径を小さくすることが可能となった。結晶粒径は、透過型電子顕微鏡(TEM)により、100個の粒子の観察を行い、粒径の平均値及び分散を求めた。結晶粒径が小さくなると、記録時のノイズが低減できる。最短で25nmのビット長の記録を行う場合、最短ビット長の半分である12.5nm以上の結晶粒が存在すると、記録時のノイズが急激に増加する。このため、結晶粒径の分散が約20%であるから、平均粒径は11.4nm以下であることが好ましい。また、Bを添加しすぎると加熱時に記録層の劣化が生じる。実際に記録を行う際の媒体の加熱時間は数nsであるが、加速試験として400℃で1h加熱した際の飽和磁化の劣化を調べた。劣化量が大きいと、書換え可能回数が少なくなるため、200emu/cc以下であることが好ましい。強磁性金属層中の硼素(B)量が異なるターゲットを用意し、強磁性金属層の膜厚を0.2nm、非磁性金属層の膜厚を0.6nm、記録層の総膜厚を12nmとして、強磁性金属層中のB添加量の異なる記録層を製膜し、膜中の硼素量と結晶粒径及び加速試験時の飽和磁化劣化量を調べたところ、図8及び表8に示すような結果が得られた。 Furthermore, it has become possible to reduce the crystal grain size by adding B (boron) into the ferromagnetic metal layer. As for the crystal grain size, 100 particles were observed with a transmission electron microscope (TEM), and the average value and dispersion of the grain size were obtained. When the crystal grain size is reduced, noise during recording can be reduced. When recording with a bit length of 25 nm at the shortest, if there is a crystal grain of 12.5 nm or more, which is half of the shortest bit length, noise during recording increases rapidly. For this reason, since the dispersion of the crystal grain size is about 20%, the average grain size is preferably 11.4 nm or less. On the other hand, if B is added too much, the recording layer deteriorates during heating. Although the heating time of the medium during actual recording is several ns, the deterioration of the saturation magnetization when heated at 400 ° C. for 1 h was examined as an acceleration test. When the amount of deterioration is large, the number of rewritable times decreases, and therefore it is preferably 200 emu / cc or less. Prepare targets with different boron (B) contents in the ferromagnetic metal layer, the ferromagnetic metal layer thickness is 0.2 nm, the nonmagnetic metal layer thickness is 0.6 nm, and the total recording layer thickness is 12 nm. As shown in FIG. 8 and Table 8, when recording layers having different B addition amounts in the ferromagnetic metal layer were formed and the boron content and crystal grain size in the film and the saturation magnetization deterioration amount during the acceleration test were examined. The result was obtained.
           表8
番号   硼素量   飽和磁化劣化量   結晶粒径
    (原子%)  (emu/cc)   (nm) 
81    0      20      12.5
82    5      20      11.0
83    8      30      10.8
84   10      50      10.6
85   13     100      10.5
86   15     180      10.3
87   19     250      10.2
Table 8
Number Boron amount Saturation magnetization deterioration Crystal grain size
(Atom%) (emu / cc) (nm)
81 0 20 12.5
82 5 20 11.0
83 8 30 10.8
84 10 50 10.6
85 13 100 10.5
86 15 180 10.3
87 19 250 10.2
 これより、強磁性金属層中の硼素量が増加するほど、飽和磁化劣化量は大きく、結晶粒径は小さくなることがわかる。強磁性金属層中の硼素量が5原子%以上15原子%以下の場合に、飽和磁化劣化量は200emu/cc以下、結晶粒径は11nm以下に出来、良好な結果が得られた。さらに、硼素量が8原子%以上13原子%以下の場合に、飽和磁化劣化量は100emu/cc以下、結晶粒径は10.8nm以下に出来、より良好な結果が得られた。 From this, it can be seen that as the amount of boron in the ferromagnetic metal layer increases, the amount of saturation magnetization deterioration increases and the crystal grain size decreases. When the boron content in the ferromagnetic metal layer was 5 atomic% or more and 15 atomic% or less, the saturation magnetization deterioration amount could be 200 emu / cc or less, the crystal grain size could be 11 nm or less, and good results were obtained. Further, when the boron content is 8 atomic% or more and 13 atomic% or less, the saturation magnetization deterioration amount can be 100 emu / cc or less and the crystal grain size can be 10.8 nm or less, and a better result is obtained.
 次に、記録層のキュリー温度と浮上特性、記録特性の関係を調べた。浮上特性は、加速試験とし、媒体にファーフィールドのレーザ光(波長780nm、スポット径1μm)を10ns、1000回照射した後、前記グライドテスタで浮上時にグライドヘッドがヒットする回数を調べた。記録特性は、近接場光でビット長50nmで記録を行い、記録ドメイン100個を磁気顕微鏡(MFM)で観察し、ビット長分散を求めた。記録パワーを変えながら測定を各媒体の最適パワーでの分散を比較した。表9に結果を纏めた。 Next, the relationship between the Curie temperature of the recording layer, the flying characteristics, and the recording characteristics was examined. As for the flying characteristics, an acceleration test was conducted, and the number of times the glide head hits when flying with the glide tester after irradiating the medium with far-field laser light (wavelength 780 nm, spot diameter 1 μm) 10 ns for 1000 times. As for the recording characteristics, recording was performed with near-field light at a bit length of 50 nm, and 100 recording domains were observed with a magnetic microscope (MFM) to determine the bit length dispersion. The measurement was compared with the dispersion at the optimum power of each medium while changing the recording power. Table 9 summarizes the results.

              表9
番号 キュリー温度(℃) ヘッドのヒット数(回) ビット長分散(%)
91    200        0         25
92    220        0         14
93    240        0         10
94    300        1          8
95    370        2          6
96    400        5          6
97    450       10          6

Table 9
Number Curie temperature (° C) Number of head hits (times) Bit length dispersion (%)
91 200 0 25
92 220 0 14
93 240 0 10
94 300 1 8
95 370 2 6
96 400 5 6
97 450 10 6
 これより、記録層のキュリー温度が高くなるほど、ヘッドのヒット数が増えることがわかる。これは、キュリー温度が高いため、記録時に記録層の温度を高くしないと記録が出来ず、この際の熱で保護層や潤滑材が熱劣化したためである。表面に凹凸が形成され、浮上特性が劣化、ヒットの回数が増加していると考えられる。また、記録層のキュリー温度が低くなるほど、ビット長分散が大きくなる。これは、記録時の温度が低い、つまり出射パワーが低く室温との差が小さくなるため、温度制御のばらつきが増加しているためである。記録層キュリー温度が220℃以上400℃以下の場合に、ヘッドのヒット数は5回以下と少なく、ビット長分散が15%以下の、良好な結果が得られた。さらに、記録層キュリー温度が250℃以上370℃以下の場合に、ヘッドのヒット数は2回以下ときわめて少なく、ビット長分散が10%以下の、より良好な結果が得られた。 From this, it can be seen that the higher the Curie temperature of the recording layer, the greater the number of head hits. This is because, since the Curie temperature is high, recording cannot be performed unless the temperature of the recording layer is increased during recording, and the protective layer and the lubricant are thermally deteriorated by the heat at this time. It is considered that irregularities are formed on the surface, the floating characteristics are deteriorated, and the number of hits is increased. Further, the lower the Curie temperature of the recording layer, the larger the bit length dispersion. This is because the temperature at the time of recording is low, that is, the output power is low and the difference from room temperature is small, so that the variation in temperature control increases. When the recording layer Curie temperature was 220 ° C. or higher and 400 ° C. or lower, the number of head hits was as small as 5 or less, and good results were obtained with a bit length dispersion of 15% or less. Further, when the recording layer Curie temperature was 250 ° C. or higher and 370 ° C. or lower, the number of hits of the head was very small, 2 times or less, and a better result was obtained with a bit length dispersion of 10% or less.
 記録層の膜厚と温度特性、磁気特性の関係を調べた。結果を表10に示す。温度特性は、記録層のエネルギー入射側(上面)とその反対の基板側(下面)の温度の差を調べた。温度差が大きいと、記録のために記録層がエネルギー照射された際に、上面だけ加熱により垂直磁気異方性が低下し磁化反転するが、下面は温度が低く垂直磁気異方性が高いままのため磁化反転せず、記録ビットが形成されない割合が増加する。従って、記録層上下間の温度差は記録温度に対して十分小さい125℃以下であることが好ましい。磁気特性としては、磁気モーメントの大きさをノミナルの記録層12nmを1としてその比で示した。磁気モーメントが低くなると、信号強度が劣化するため、磁気モーメントの大きさはノミナルの0.5以上が必要である。 The relationship between the film thickness of the recording layer, temperature characteristics, and magnetic characteristics was examined. The results are shown in Table 10. As for the temperature characteristics, the temperature difference between the energy incident side (upper surface) of the recording layer and the opposite substrate side (lower surface) was examined. When the temperature difference is large, when the recording layer is irradiated with energy for recording, the perpendicular magnetic anisotropy is decreased by heating only the upper surface and the magnetization is reversed, but the lower surface remains low in temperature and high in perpendicular magnetic anisotropy. For this reason, magnetization reversal does not occur, and the rate at which recording bits are not formed increases. Therefore, the temperature difference between the upper and lower recording layers is preferably 125 ° C. or less, which is sufficiently small with respect to the recording temperature. As the magnetic characteristics, the magnitude of the magnetic moment is shown as a ratio with the nominal recording layer 12 nm being 1. When the magnetic moment is lowered, the signal strength is deteriorated. Therefore, the magnitude of the magnetic moment needs to be 0.5 or more of the nominal value.

              表10
番号   記録層膜厚  記録層上下間の温度差  磁気モーメント
      (nm)     (℃)              
101    4        5        0.3
102    6       20        0.5
103    8.4     45        0.7
104   12       90        1
105   13      105        1.1
106   15      125        1.25
107   18      153        1.5

Table 10
Number Recording layer thickness Temperature difference between upper and lower recording layers Magnetic moment
(Nm) (℃)
101 4 5 0.3
102 6 20 0.5
103 8.4 45 0.7
104 12 90 1
105 13 105 1.1
106 15 125 1.25
107 18 153 1.5
 表10より、記録層膜厚が厚くなるほど、記録層上下間の温度差が広がることがわかる。これは、近接場光が光源からはなれたところでは、光強度が低下するためであり。また、記録層膜厚が薄くなるほど、磁気モーメントが小さくなる。これは、記録層の磁化とその体積に関係しているためである。記録層膜厚が6nm以上15nm以下の場合に、記録層上下間の温度差は125℃、磁気モーメント0.5以上の、良好な結果が得られた。さらに、記録層膜厚が8.4nm以上13nm以下の場合に、記録層上下間の温度差は105℃、磁気モーメント0.7以上の、より良好な結果が得られた。 Table 10 shows that the temperature difference between the upper and lower recording layers increases as the recording layer thickness increases. This is because the light intensity decreases where the near-field light is separated from the light source. In addition, the magnetic moment decreases as the recording layer thickness decreases. This is because it is related to the magnetization of the recording layer and its volume. When the thickness of the recording layer was 6 nm or more and 15 nm or less, good results were obtained in which the temperature difference between the upper and lower recording layers was 125 ° C. and the magnetic moment was 0.5 or more. Furthermore, when the recording layer thickness was 8.4 nm or more and 13 nm or less, a better result was obtained in which the temperature difference between the upper and lower recording layers was 105 ° C. and the magnetic moment was 0.7 or more.
[実施例2]
 実施例2では、本発明の一つの実施例として、室温で垂直磁気異方性を有する磁気記録層とキャップ層を有し、エネルギー照射(アシスト)により垂直磁気異方性を低下させた状態で記録を行う垂直磁気記録媒体を説明する。
[Example 2]
In Example 2, as one example of the present invention, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature and a cap layer are provided, and the perpendicular magnetic anisotropy is lowered by energy irradiation (assist). A perpendicular magnetic recording medium for recording will be described.
 図9(a)は、本発明の一実施例として、強磁性金属層108と非磁性金属層109の多層膜からなる記録層104と、キャップ層用強磁性金属層901とキャップ層用非磁性金属層902の多層膜からなるキャップ層105を有する垂直磁気記録媒体の断面構造を模式的に示したものである。基板101上に、下地層102として約30nmのNi63Ta38層と約7nmのNi946層、中間層103として約16nmのRu層、約12nmの記録層104、約3nmのキャップ層105、保護層106として約3nmのCN層を順次形成した。製膜は、それぞれDCスパッタリングにて行った。その後、CN層の上に、約1nmの潤滑材107を塗布した。 FIG. 9A shows a recording layer 104 composed of a multilayer film of a ferromagnetic metal layer 108 and a nonmagnetic metal layer 109, a cap layer ferromagnetic metal layer 901, and a cap layer nonmagnetic as an embodiment of the present invention. 1 schematically shows a cross-sectional structure of a perpendicular magnetic recording medium having a cap layer 105 formed of a multilayer film of metal layers 902. On the substrate 101, a Ni 63 Ta 38 layer and a Ni 94 W 6 layer of about 30 nm as the underlayer 102, a Ru layer of about 16 nm as the intermediate layer 103, a recording layer 104 of about 12 nm, and a cap layer 105 of about 3 nm. Then, a CN layer of about 3 nm was sequentially formed as the protective layer 106. Film formation was performed by DC sputtering. Thereafter, about 107 nm of the lubricant 107 was applied on the CN layer.
 記録層104は、強磁性金属層108にはCo9010を0.2nm、非磁性金属層109にはPdを0.6nmを用いて積層し、微量の酸素を添加した。詳細は実施例1に記載の通りである。図9(b)は、キャップ層105を拡大したものである。キャップ層105は、キャップ層用強磁性金属層901にはCoを0.2nm、キャップ層用非磁性金属層902にはPdを0.6nmを用いて積層した。積層数はキャップ層3nmの場合、約4回である。多層膜構造のキャップ層の形成は、基板を固定し、CoのターゲットとPdターゲットを回転させながら、両層を交互に形成して行った。ターゲットを固定し、基板を回転させても同様の多層膜が形成できる。各構成層の膜厚は、各ターゲットに投入するパワーを変えることにより、変化させた。キャップ層製膜時のガス圧は5Paにした。 The recording layer 104 was laminated using Co 90 B 10 of 0.2 nm for the ferromagnetic metal layer 108 and Pd of 0.6 nm for the nonmagnetic metal layer 109, and a trace amount of oxygen was added. Details are as described in Example 1. FIG. 9B is an enlarged view of the cap layer 105. The cap layer 105 was laminated by using 0.2 nm of Co for the ferromagnetic metal layer 901 for the cap layer and 0.6 nm of Pd for the nonmagnetic metal layer 902 for the cap layer. When the cap layer is 3 nm, the number of layers is about 4 times. The cap layer having the multilayer structure was formed by alternately forming both layers while fixing the substrate and rotating the Co target and the Pd target. A similar multilayer film can be formed by fixing the target and rotating the substrate. The film thickness of each constituent layer was changed by changing the power input to each target. The gas pressure during cap layer deposition was 5 Pa.
 比較例には、上記キャップ層の組成と構造のみ異なる媒体を作製し、浮上特性及び磁気特性の比較を行った。キャップ層に、Co65Cr15Pt128組成を用いて、比較した。 In the comparative example, media different in composition and structure of the cap layer were prepared, and the flying characteristics and magnetic characteristics were compared. A comparison was made using a Co 65 Cr 15 Pt 12 B 8 composition for the cap layer.
 まず、多層膜構造のキャップ層及び比較のキャップ層を有する媒体を形成し、垂直磁気記録媒体の浮上特性を調べ、表11にて比較した。ここでは、浮上特性が良好な媒体が得られる歩留まりを調べた。歩留まりは、同様の構成の媒体を20枚作製し、前記ピエゾ出力が31.3mV以下のものをA級品、31.4から31.5mVのものをB級品、31.6mV以上のものをNGとしてカウントして、各割合を調べた。 First, a medium having a multi-layered cap layer and a comparative cap layer was formed, and the flying characteristics of the perpendicular magnetic recording medium were examined and compared in Table 11. Here, the yield at which a medium with good flying characteristics was obtained was examined. For the yield, 20 media having the same configuration were prepared, and those with a piezoelectric output of 31.3 mV or less were Class A products, those with 31.4 to 31.5 mV were Class B products, and those with 31.6 mV or more were used. Each percentage was examined by counting as NG.
Figure JPOXMLDOC01-appb-T000001
Figure JPOXMLDOC01-appb-T000001
 表11より、キャップ層が厚いほど歩留まりが増加することがわかる。キャップ層厚さ1nm以上の場合に、A級品歩留まりは90%と、良好な結果が得られた。さらに、キャップ層厚さ2nm以上の場合に、A級品歩留まりは95%に向上し、より良好な結果が得られた。浮上特性の向上は、多層膜キャップ層でも比較例のキャップ層でも同様に向上した。浮上特性が向上した理由は、図10に示されるように、記録層表面に結晶粒形成により形成された凹凸をキャップ層105の形成により滑らかに出来たためと考えられる。 From Table 11, it can be seen that the thicker the cap layer, the higher the yield. When the cap layer thickness was 1 nm or more, the A-class product yield was 90%, and good results were obtained. Furthermore, when the cap layer thickness was 2 nm or more, the yield of Class A products was improved to 95%, and better results were obtained. The improvement of the flying characteristics was similarly improved in both the multilayer cap layer and the comparative cap layer. The reason why the flying characteristics are improved is considered to be that the unevenness formed by the formation of crystal grains on the surface of the recording layer was made smooth by forming the cap layer 105 as shown in FIG.
 次に、磁気特性の比較を行った。各媒体の保磁力を測定し、キャップ層形成による保磁力の劣化量を調べた。本発明と比較例にそれぞれキャップ層を形成した場合の磁気特性を、図11及び表11で比較した。多層化されていない、Co65Cr15Pt128組成のキャップ層を有する比較例では、保磁力劣化が極めて大きく、1nm形成しただけでも2kOe以上という大きな劣化を示した。これは、保磁力の大きな記録層上に保磁力の小さなキャップ層が形成されたため、媒体全体の磁気特性が劣化したためである。一方、本発明の多層膜キャップ層付媒体では、浮上特性を向上するためにキャップ層を形成しても磁気特性の劣化はきわめて小さく、4nmキャップ層を形成しても1.5kOeと劣化が小さいことがわかる。これは、キャップ層も多層膜構造とすることで保磁力の大きな層を重ねた構成にしたためと考えられる。このように、高い垂直磁気異方性を持つ記録層にキャップ層用強磁性金属層とキャップ層用非磁性金属層からなる多層膜構造のキャップ層を設けることで、磁気特性の劣化を防ぎかつ、浮上特性を極めて良好にすることが可能となった。 Next, the magnetic characteristics were compared. The coercive force of each medium was measured, and the amount of coercive force deterioration due to cap layer formation was examined. The magnetic characteristics when the cap layer is formed in the present invention and the comparative example are compared in FIG. In the comparative example having a Co 65 Cr 15 Pt 12 B 8 composition cap layer that is not multi-layered, the coercive force deterioration was extremely large, and even when 1 nm was formed, a large deterioration of 2 kOe or more was shown. This is because the cap layer having a small coercive force was formed on the recording layer having a large coercive force, so that the magnetic characteristics of the entire medium deteriorated. On the other hand, in the medium with a multilayer film cap layer of the present invention, even if a cap layer is formed to improve the floating characteristics, the deterioration of magnetic characteristics is extremely small, and even if a 4 nm cap layer is formed, the deterioration is as small as 1.5 kOe. I understand that. This is presumably because the cap layer also has a multilayer film structure so that layers having a large coercive force are stacked. Thus, by providing a cap layer having a multilayer structure comprising a ferromagnetic metal layer for a cap layer and a nonmagnetic metal layer for a cap layer on a recording layer having a high perpendicular magnetic anisotropy, it is possible to prevent deterioration of magnetic characteristics and As a result, the flying characteristics can be made extremely good.
 さらに、記録層等の条件を一定にしたまま、多層膜キャップ層の組成、プロセス依存性を調べ、表12に示した。キャップ層用強磁性金属層901にはCo9010を0.2nm、キャップ層用非磁性金属層902にはPdを0.6nmを用いて積層した媒体を作製した(番号121)。キャップ層の厚さは2nmとした。このようにBを添加した場合、A級品の歩留まりは85%に低下した。これより、キャップ層にはBを添加しない方が良いことがわかった。 Further, the composition and process dependency of the multilayer cap layer were investigated while keeping the conditions of the recording layer, etc., and are shown in Table 12. A medium in which Co 90 B 10 is 0.2 nm for the ferromagnetic metal layer 901 for the cap layer and Pd is 0.6 nm for the nonmagnetic metal layer 902 for the cap layer was manufactured (No. 121). The thickness of the cap layer was 2 nm. When B was added in this way, the yield of Class A products decreased to 85%. From this, it was found that it is better not to add B to the cap layer.
 キャップ層用強磁性金属層901にはCoを0.2nm、キャップ層用非磁性金属層902にはPdを0.6nmを用いて積層した媒体を作製した。ここでは記録層同様、微量の酸素添加を行った。酸素添加をした場合、キャップ層中のO量が10原子%のとき(番号122)、A級品の歩留まりは80%に低下した。キャップ層中のO量が5原子%のとき(番号123)、A級品の歩留まりは85%であった。これより、キャップ層中の酸素量は少ないほうが良いことがわかった。 A medium in which the ferromagnetic metal layer 901 for the cap layer was laminated using Co of 0.2 nm and the nonmagnetic metal layer 902 for the cap layer was laminated using 0.6 nm of Pd was produced. Here, as with the recording layer, a small amount of oxygen was added. In the case where oxygen was added, when the amount of O in the cap layer was 10 atomic% (No. 122), the yield of the class A product decreased to 80%. When the amount of O in the cap layer was 5 atomic% (No. 123), the yield of the class A product was 85%. From this, it was found that a smaller amount of oxygen in the cap layer is better.
 キャップ層用強磁性金属層901にはCo9010を0.1nm、キャップ層用非磁性金属層902にはPdを0.6nmを用いて積層した媒体(番号124)を作製した。キャップ層の厚さは2nmとした。このような強磁性金属層を記録層より薄くした場合、A級品の歩留まりは95%のままで保磁力の劣化が低減できることがわかった。 A medium (No. 124) was prepared by laminating Co 90 B 10 with 0.1 nm for the cap layer ferromagnetic metal layer 901 and Pd with 0.6 nm for the non-magnetic metal layer 902 for cap layer. The thickness of the cap layer was 2 nm. It has been found that when such a ferromagnetic metal layer is made thinner than the recording layer, the degradation of the coercive force can be reduced while the yield of the class A product remains 95%.
 キャップ層用強磁性金属層901にはCoを0.1nm、キャップ層用非磁性金属層902にはPdを0.6nmを用いて積層した媒体(番号125)を作製した。キャップ層の厚さは2nmとした。このように強磁性金属層にBを入れず、さらに構成層を記録層より薄くした場合、A級品の歩留まりは97%に向上し、さらに保磁力の劣化が低減できることがわかった。 A medium (No. 125) was prepared by laminating Co for the cap layer ferromagnetic metal layer 901 with 0.1 nm of Co and for the cap layer nonmagnetic metal layer 902 with Pd of 0.6 nm. The thickness of the cap layer was 2 nm. Thus, it was found that when B was not added to the ferromagnetic metal layer and the constituent layer was made thinner than the recording layer, the yield of the class A product was improved to 97% and the coercive force deterioration could be further reduced.
 キャップ層用強磁性金属層901にはCo9010を0.2nm、キャップ層用非磁性金属層902にはPdを0.6nmを用いて、スパッタリングガス圧を3.5Paで積層した媒体(番号126)を作製した。キャップ層の厚さは2nmとした。このようにガス圧を下げると、製膜レートが高くなり量産性が向上する。A級品の歩留まりも95%のままで、保磁力の劣化は少し大きくなった。 A medium in which Co 90 B 10 is 0.2 nm for the ferromagnetic metal layer 901 for the cap layer, Pd is 0.6 nm for the non-magnetic metal layer 902 for the cap layer, and the sputtering gas pressure is 3.5 Pa. No. 126) was produced. The thickness of the cap layer was 2 nm. When the gas pressure is lowered in this way, the film forming rate is increased and the mass productivity is improved. The yield of class A products remained at 95%, and the coercivity deteriorated slightly.
 キャップ層用強磁性金属層901にはCoを0.2nm、キャップ層用非磁性金属層902にはPdを0.6nmを用いて、スパッタリングガス圧を3.5Paで積層した媒体(番号127)を作製した。キャップ層の厚さは2nmとした。このようにガス圧を下げると、製膜レートが高くなり量産性が向上する。A級品の歩留まりは97%に向上した。保磁力の劣化は少し大きくなった。 A medium (No. 127) in which Co is 0.2 nm for the ferromagnetic metal layer 901 for the cap layer, Pd is 0.6 nm for the nonmagnetic metal layer 902 for the cap layer, and the sputtering gas pressure is 3.5 Pa. Was made. The thickness of the cap layer was 2 nm. When the gas pressure is lowered in this way, the film forming rate is increased and the mass productivity is improved. The yield of Class A products improved to 97%. The degradation of the coercive force was slightly increased.

         表12
番号    A級品(%)  保磁力劣化量(kOe)
114    95      0.8
121    85      0.8
122    80      0.8
123    85      0.8
124    95      0.6
125    97      0.6
126    95      0.9
127    97      0.9

Table 12
Number Class A product (%) Coercive force degradation (kOe)
114 95 0.8
121 85 0.8
122 80 0.8
123 85 0.8
124 95 0.6
125 97 0.6
126 95 0.9
127 97 0.9
 なお、本実施例に記載していない層構成、製造方法、材料、評価方法等は実施例1と同様にした。 The layer configuration, manufacturing method, material, evaluation method, etc. not described in this example were the same as in Example 1.
[実施例3]
 本発明の一実施例である磁気記憶装置の概略を図12に示した。(a)は平面模式図、(b)はそのA-A’断面図である。(c)はヘッドの概略図、(d)はヘッド主要部の側面からみた概略図である。
[Example 3]
An outline of a magnetic memory device according to an embodiment of the present invention is shown in FIG. (A) is a schematic plan view, and (b) is an AA ′ sectional view thereof. (C) is a schematic diagram of the head, and (d) is a schematic diagram viewed from the side of the main part of the head.
 この装置は、垂直磁気記録媒体1501、これを駆動する駆動部1502、磁気ヘッド用浮上スライダ1503及び磁気ヘッドの駆動手段1504、磁気ヘッドの記録再生信号処理手段1505を有する。磁気ヘッドは、磁気ヘッドスライダ上に形成された記録再生分離型の磁気ヘッドであり、記録ヘッドには磁界を形成する手段1507及び近接場光を用いたエネルギー照射手段1506が設けられている。さらに磁気ヘッドには、再生電流用検出手段(再生ヘッド)1508が設けられ、記録されたビットの再生を行う。近接場光は、サスペンション1201上に形成された光導波路1202を通して、近接場光を用いたエネルギー照射手段1506に供給される。浮上スライダ1503は、位置決め精度を向上させるため、フレクシャー1203を介してサスペンションに取り付けられている。 This apparatus has a perpendicular magnetic recording medium 1501, a driving unit 1502 for driving the medium 150, a magnetic head flying slider 1503, a magnetic head driving means 1504, and a magnetic head recording / reproducing signal processing means 1505. The magnetic head is a recording / reproducing separation type magnetic head formed on a magnetic head slider. The recording head is provided with means 1507 for forming a magnetic field and energy irradiation means 1506 using near-field light. Further, the magnetic head is provided with a reproducing current detecting means (reproducing head) 1508 to reproduce the recorded bit. Near-field light is supplied to an energy irradiation means 1506 using near-field light through an optical waveguide 1202 formed on the suspension 1201. The flying slider 1503 is attached to the suspension via the flexure 1203 in order to improve positioning accuracy.
 次に、記録時の熱や磁気特性について調べた。光源波長は780nmであり、垂直磁気記録媒体1501には図1に記載の構造を用いた。図13に、エネルギー照射源である近接場光源から記録層表面までの距離(磁気スペーシング)と垂直磁気記録媒体におけるエネルギー吸収率の関係を調べた。これは、近接場光の強度とその波長における媒体の吸収率から算出し、当該距離が4nmの場合を1とし規格化した。これより、当該距離が小さいほど媒体の吸収率が大きいことがわかる。吸収率が小さい場合、近接場光では十分媒体を加熱することが出来ず、記録が行えないため、吸収率は25%以上が好ましい。エネルギー照射源から記録層表面までの距離が8nm以下の場合に、吸収率が25%以上と良好な結果が得られた。さらに、エネルギー照射源から記録層表面までの距離が7nm以下の場合に、吸収率が32%以上とより良好な結果が得られた。 Next, the thermal and magnetic characteristics during recording were examined. The light source wavelength is 780 nm, and the perpendicular magnetic recording medium 1501 has the structure shown in FIG. FIG. 13 shows the relationship between the distance (magnetic spacing) from the near-field light source, which is the energy irradiation source, to the recording layer surface and the energy absorption rate in the perpendicular magnetic recording medium. This was calculated from the intensity of near-field light and the absorptance of the medium at that wavelength, and normalized when the distance was 4 nm. From this, it can be seen that the smaller the distance, the larger the absorption rate of the medium. When the absorptance is small, the medium cannot be heated sufficiently with near-field light and recording cannot be performed. Therefore, the absorptance is preferably 25% or more. When the distance from the energy irradiation source to the recording layer surface was 8 nm or less, an absorptivity of 25% or more was obtained. Furthermore, when the distance from the energy irradiation source to the surface of the recording layer was 7 nm or less, an absorptivity was 32% or more and a better result was obtained.
 さらに、実施例1に記載した媒体を上記磁気記憶装置に組み込んで、ヘッド浮上量4nmで安定にヘッドが浮上することを確認したのち、上記近接場光を用いたエネルギー照射手段を搭載したヘッドを用いて記録を行った。MFMにてドメインを評価したところ、線密度方向は約25nm、トラック幅方向は50nmのドメインが形成できたことがわかった。 Furthermore, after incorporating the medium described in Example 1 into the magnetic storage device and confirming that the head stably floats at a head flying height of 4 nm, a head equipped with the energy irradiation means using the near-field light is mounted. And recorded. When the domain was evaluated by MFM, it was found that a domain having a linear density direction of about 25 nm and a track width direction of 50 nm could be formed.
 以上から、基板と、基板上に設けられた下地層及び中間層と、室温で垂直磁気異方性を有する磁気記録層と保護層を有し、エネルギー照射により垂直磁気異方性を低下させた状態で記録を行う垂直磁気記録媒体として、中間層をRu及び/又はPdで形成し、磁気記録層を、Coを主成分とする強磁性金属層とPdを主成分とする非磁性金属層との積層体で構成し、強磁性金属層の膜厚を0.15nm以上0.25nm以下とし、非磁性金属層の膜厚を0.45nm以上0.8nm以下とし、強磁性金属層と非磁性金属層の膜厚比を2以上4以下とし、エネルギー照射時と非照射時の保磁力の差を8kOe以上とした垂直磁気記録媒体を備え、更に近接場光を用いたエネルギー照射機能を有する磁気記録用ヘッドと信号再生用ヘッドとを備え、記録時のエネルギー照射源から磁気記録層表面までの距離を8nm以下とすることにより、良好な記録再生特性を有するエネルギーアシスト型磁気記憶装置を得ることができる。 From the above, it has a substrate, an underlayer and an intermediate layer provided on the substrate, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature, and a protective layer, and the perpendicular magnetic anisotropy is lowered by energy irradiation. As a perpendicular magnetic recording medium for recording in a state, an intermediate layer is formed of Ru and / or Pd, and a magnetic recording layer is composed of a ferromagnetic metal layer mainly containing Co and a nonmagnetic metal layer mainly containing Pd. The ferromagnetic metal layer has a thickness of 0.15 nm to 0.25 nm, the nonmagnetic metal layer has a thickness of 0.45 nm to 0.8 nm, and the ferromagnetic metal layer is nonmagnetic. A magnetic layer having a metal layer thickness ratio of 2 to 4 and a perpendicular magnetic recording medium in which the difference in coercivity between energy irradiation and non-irradiation is 8 kOe or more, and further has an energy irradiation function using near-field light. Includes a recording head and a signal playback head , The distance from the energy radiation source during recording to the magnetic recording layer surface by a 8nm or less, it is possible to obtain an energy-assisted magnetic memory device having good recording and reproduction characteristics.
101 基板
102 下地層
103 中間層
104 記録層
105 キャップ層
106 保護層
107 潤滑材
108 強磁性金属層
109 非磁性金属層
201 第1中間層
202 第2中間層
203 結晶粒
204 粒界
901 キャップ層用強磁性金属層
902 キャップ層用非磁性金属層
1201 サスペンション
1202 光導波路
1203 フレクシャー
1501 垂直磁気記録媒体
1502 媒体駆動部
1503 浮上スライダ
1504 磁気ヘッド駆動手段
1505 記録再生信号処理手段
1506 近接場光を用いたエネルギー照射手段
1507 磁界を形成する手段
1508 再生ヘッド
101 Substrate 102 Underlayer 103 Intermediate layer 104 Recording layer 105 Cap layer 106 Protective layer 107 Lubricant 108 Ferromagnetic metal layer 109 Nonmagnetic metal layer 201 First intermediate layer 202 Second intermediate layer 203 Crystal grain 204 Grain boundary 901 For cap layer Ferromagnetic metal layer 902 Non-magnetic metal layer for cap layer 1201 Suspension 1202 Optical waveguide 1203 Flexure 1501 Perpendicular magnetic recording medium 1502 Medium drive unit 1503 Flying slider 1504 Magnetic head drive means 1505 Recording / reproduction signal processing means 1506 Energy using near-field light Irradiation means 1507 Means 1508 for forming a magnetic field Reproducing head

Claims (12)

  1.  基板と、該基板上に設けられた下地層及び中間層と、室温で垂直磁気異方性を有する磁気記録層と保護層を有し、エネルギー照射により前記磁気記録層の垂直磁気異方性を低下させた状態で記録を行う垂直磁気記録媒体であって、
     前記中間層がRu及び/又はPdからなり、
     前記磁気記録層は、Coを主成分とする強磁性金属層とPdを主成分とする非磁性金属層との積層体であり、
     前記強磁性金属層の膜厚が0.15nm以上0.25nm以下であり、
     前記非磁性金属層の膜厚が0.45nm以上0.8nm以下であり、
     前記強磁性金属層と前記非磁性金属層の膜厚比が2以上4以下であり、
     前記エネルギー照射時と非照射時の保磁力の差が8kOe以上あることを特徴とする垂直磁気記録媒体。
    A substrate, an underlayer and an intermediate layer provided on the substrate, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature, and a protective layer, and the perpendicular magnetic anisotropy of the magnetic recording layer by energy irradiation; A perpendicular magnetic recording medium for recording in a lowered state,
    The intermediate layer is made of Ru and / or Pd;
    The magnetic recording layer is a laminate of a ferromagnetic metal layer mainly containing Co and a nonmagnetic metal layer mainly containing Pd,
    The ferromagnetic metal layer has a thickness of 0.15 nm or more and 0.25 nm or less,
    The nonmagnetic metal layer has a thickness of 0.45 nm or more and 0.8 nm or less,
    The film thickness ratio of the ferromagnetic metal layer and the nonmagnetic metal layer is 2 or more and 4 or less,
    A perpendicular magnetic recording medium characterized in that a difference in coercive force between energy irradiation and non-irradiation is 8 kOe or more.
  2.  基板と、該基板上に設けられた下地層及び中間層と、室温で垂直磁気異方性を有する磁気記録層とキャップ層と保護層を有し、エネルギー照射により前記磁気記録層の垂直磁気異方性を低下させた状態で記録を行う垂直磁気記録媒体であって、
     前記中間層がRu及び/又はPdからなり、
     前記磁気記録層は、Coを主成分とする強磁性金属層とPdを主成分とする非磁性金属層との積層体であり、
     前記キャップ層がCoを主成分とする強磁性金属層とPdを主成分とする非磁性金属層との積層体からなり、
     前記強磁性金属層の膜厚が0.15nm以上0.25nm以下であり、
     前記非磁性金属層の膜厚が0.45nm以上0.8nm以下であり、
     前記強磁性金属層と前記非磁性金属層の膜厚比が2以上4以下であり、
     前記エネルギー照射時と非照射時の保磁力の差が8kOe以上あることを特徴とする垂直磁気記録媒体。
    A substrate, an underlayer and an intermediate layer provided on the substrate, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature, a cap layer, and a protective layer. A perpendicular magnetic recording medium that performs recording in a state of reduced directionality,
    The intermediate layer is made of Ru and / or Pd;
    The magnetic recording layer is a laminate of a ferromagnetic metal layer mainly containing Co and a nonmagnetic metal layer mainly containing Pd,
    The cap layer comprises a laminate of a ferromagnetic metal layer mainly composed of Co and a nonmagnetic metal layer mainly composed of Pd,
    The ferromagnetic metal layer has a thickness of 0.15 nm or more and 0.25 nm or less,
    The nonmagnetic metal layer has a thickness of 0.45 nm or more and 0.8 nm or less,
    The film thickness ratio of the ferromagnetic metal layer and the nonmagnetic metal layer is 2 or more and 4 or less,
    A perpendicular magnetic recording medium characterized in that a difference in coercive force between energy irradiation and non-irradiation is 8 kOe or more.
  3.  前記磁気記録層のキュリー温度が220℃以上400℃以下であることを特徴とする、請求項1又は2に記載の垂直磁気記録媒体。 The perpendicular magnetic recording medium according to claim 1, wherein the magnetic recording layer has a Curie temperature of 220 ° C. or more and 400 ° C. or less.
  4.  前記磁気記録層中の平均酸素濃度が5原子%以上15原子%以下であることを特徴とする、請求項1又は2に記載の垂直磁気記録媒体。 3. The perpendicular magnetic recording medium according to claim 1, wherein an average oxygen concentration in the magnetic recording layer is 5 atomic% or more and 15 atomic% or less.
  5.  前記強磁性金属層中の平均硼素濃度が5原子%以上15原子%以下であることを特徴とする、請求項1又は2に記載の垂直磁気記録媒体。 3. The perpendicular magnetic recording medium according to claim 1, wherein an average boron concentration in the ferromagnetic metal layer is 5 atomic% or more and 15 atomic% or less.
  6.  前記磁気記録層の膜厚が6nm以上15nm以下であることを特徴とする、請求項1又は2に記載の垂直磁気記録媒体。 The perpendicular magnetic recording medium according to claim 1, wherein the magnetic recording layer has a thickness of 6 nm to 15 nm.
  7.  前記キャップ層中の平均酸素濃度が前記磁気記録層の平均酸素濃度より低いことを特徴とする、請求項2に記載の垂直磁気記録媒体。 3. The perpendicular magnetic recording medium according to claim 2, wherein an average oxygen concentration in the cap layer is lower than an average oxygen concentration in the magnetic recording layer.
  8.  前記キャップ層の膜厚が1nm以上4nm以下であることを特徴とする、請求項2に記載の垂直磁気記録媒体。 The perpendicular magnetic recording medium according to claim 2, wherein the cap layer has a thickness of 1 nm to 4 nm.
  9.  前記中間層がPdからなることを特徴とする請求項1又は2に記載の垂直磁気記録媒体。 3. The perpendicular magnetic recording medium according to claim 1, wherein the intermediate layer is made of Pd.
  10.  前記中間層がRuからなることを特徴とする請求項1又は2に記載の垂直磁気記録媒体。 3. The perpendicular magnetic recording medium according to claim 1, wherein the intermediate layer is made of Ru.
  11.  前記中間層がRuとPdからなることを特徴とする請求項1又は2に記載の垂直磁気記録媒体。 3. The perpendicular magnetic recording medium according to claim 1, wherein the intermediate layer is made of Ru and Pd.
  12.  基板と、該基板上に設けられた下地層及び中間層と、室温で垂直磁気異方性を有する磁気記録層と保護層を有し、エネルギー照射により前記磁気記録層の垂直磁気異方性を低下させた状態で記録を行う垂直磁気記録媒体と、
     近接場光を用いたエネルギー照射機能を有する磁気記録用ヘッドと信号再生用ヘッドとを有する磁気ヘッドと備え、
     前記垂直磁気記録媒体は、前記中間層がRu及び/又はPdからなり、前記磁気記録層は、Coを主成分とする強磁性金属層とPdを主成分とする非磁性金属層との積層体であり、前記強磁性金属層の膜厚が0.15nm以上0.25nm以下であり、前記非磁性金属層の膜厚が0.45nm以上0.8nm以下であり、前記強磁性金属層と非磁性金属層の膜厚比が2以上4以下であり、前記エネルギー照射時と非照射時の保磁力の差が8kOe以上あり、
     記録時に前記磁気ヘッドの前記エネルギー照射源から前記垂直磁気記録媒体の前記磁気記録層表面までの距離が8nm以下であることを特徴とする磁気記憶装置。
    A substrate, an underlayer and an intermediate layer provided on the substrate, a magnetic recording layer having a perpendicular magnetic anisotropy at room temperature, and a protective layer, and the perpendicular magnetic anisotropy of the magnetic recording layer by energy irradiation; A perpendicular magnetic recording medium for recording in a lowered state;
    A magnetic head having a magnetic recording head having an energy irradiation function using near-field light and a signal reproducing head;
    In the perpendicular magnetic recording medium, the intermediate layer is made of Ru and / or Pd, and the magnetic recording layer is a laminate of a ferromagnetic metal layer mainly containing Co and a nonmagnetic metal layer mainly containing Pd. The ferromagnetic metal layer has a thickness of 0.15 nm to 0.25 nm and the nonmagnetic metal layer has a thickness of 0.45 nm to 0.8 nm. The thickness ratio of the magnetic metal layer is 2 or more and 4 or less, and the difference in coercive force between the energy irradiation and non-irradiation is 8 kOe or more,
    A magnetic storage device, wherein a distance from the energy irradiation source of the magnetic head to the surface of the magnetic recording layer of the perpendicular magnetic recording medium is 8 nm or less during recording.
PCT/JP2009/068866 2008-11-06 2009-11-05 Perpendicular magnetic recording medium and magnetic storage device WO2010053106A1 (en)

Applications Claiming Priority (2)

Application Number Priority Date Filing Date Title
JP2008285772A JP5301953B2 (en) 2008-11-06 2008-11-06 Perpendicular magnetic recording medium
JP2008-285772 2008-11-06

Publications (1)

Publication Number Publication Date
WO2010053106A1 true WO2010053106A1 (en) 2010-05-14

Family

ID=42152914

Family Applications (1)

Application Number Title Priority Date Filing Date
PCT/JP2009/068866 WO2010053106A1 (en) 2008-11-06 2009-11-05 Perpendicular magnetic recording medium and magnetic storage device

Country Status (2)

Country Link
JP (1) JP5301953B2 (en)
WO (1) WO2010053106A1 (en)

Families Citing this family (1)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
US9318140B2 (en) 2012-12-19 2016-04-19 HGST Netherlands B.V. Exchange enhanced cap manufactured with argon and oxygen implantation

Citations (3)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
JP2005038569A (en) * 2003-03-20 2005-02-10 Hitachi Maxell Ltd Magnetic recording medium, its recording method, and magnetic recording device
JP2006209903A (en) * 2005-01-31 2006-08-10 Hitachi Maxell Ltd Information recording medium
JP2008021365A (en) * 2006-07-12 2008-01-31 Hitachi Maxell Ltd Information recording medium and manufacturing method thereof, and information recording/reproducing device

Patent Citations (3)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
JP2005038569A (en) * 2003-03-20 2005-02-10 Hitachi Maxell Ltd Magnetic recording medium, its recording method, and magnetic recording device
JP2006209903A (en) * 2005-01-31 2006-08-10 Hitachi Maxell Ltd Information recording medium
JP2008021365A (en) * 2006-07-12 2008-01-31 Hitachi Maxell Ltd Information recording medium and manufacturing method thereof, and information recording/reproducing device

Also Published As

Publication number Publication date
JP2010113763A (en) 2010-05-20
JP5301953B2 (en) 2013-09-25

Similar Documents

Publication Publication Date Title
JP5153575B2 (en) Thermally assisted magnetic recording medium and magnetic recording apparatus
WO2011093233A1 (en) Heat-assisted magnetic recording medium and magnetic recording and reproducing device
US9361924B2 (en) Magnetic recording medium and magnetic recording and reproducing apparatus
US20070254189A1 (en) Magnetic storage device
US7274626B2 (en) Magneto-optical recording using a heating element
US20110020669A1 (en) Magnetic recording medium
JP7279563B2 (en) Thermally assisted magnetic recording medium and magnetic storage device
US20080292906A1 (en) Enhancement of Magnetic Media Recording Performance Using Ion Irradiation to Tailor Exchange Coupling
US6963461B2 (en) Method for magnetic recording on laminated media with improved media signal-to-noise ratio
JP3884031B2 (en) Thermally assisted magnetic recording device using near-field light
JP5301953B2 (en) Perpendicular magnetic recording medium
JP3886011B2 (en) Magnetic recording medium, recording method therefor, and magnetic recording apparatus
JP5710531B2 (en) Thermally assisted magnetic recording method and thermally assisted magnetic recording apparatus
JP4711984B2 (en) Perpendicular magnetic recording medium, magnetic storage device, and magnetic recording method
JP2007164836A (en) Magnetic recording medium and magnetic recording device
JP3908771B2 (en) Magnetic recording medium, recording method therefor, and magnetic recording apparatus
Wang et al. SNR impact of media anisotropy near curie temperature in heat-assisted magnetic recording
JP2005038587A (en) Magnetic recording disk drive having laminated medium in which signal to noise ratio is improved
JP4339266B2 (en) Information recording medium, method for manufacturing the same, information reproducing apparatus, and information recording / reproducing apparatus
JP2006147046A (en) Magnetic recording medium, method for manufacturing magnetic recording medium, and magnetic recorder
JP2005285186A (en) Manufacturing method of magnetic recording medium, and magnetic recording medium manufactured by the same method
US20200357436A1 (en) Magnetic recording medium and magnetic read/write apparatus
JP2008021365A (en) Information recording medium and manufacturing method thereof, and information recording/reproducing device
JP2008287771A (en) Perpendicular magnetic recording medium, method for manufacturing the same, and magnetic recoding device
JP2006209903A (en) Information recording medium

Legal Events

Date Code Title Description
121 Ep: the epo has been informed by wipo that ep was designated in this application

Ref document number: 09824805

Country of ref document: EP

Kind code of ref document: A1

NENP Non-entry into the national phase

Ref country code: DE

122 Ep: pct application non-entry in european phase

Ref document number: 09824805

Country of ref document: EP

Kind code of ref document: A1