CA2188150A1 - Improved disk substrate - Google Patents

Improved disk substrate

Info

Publication number
CA2188150A1
CA2188150A1 CA002188150A CA2188150A CA2188150A1 CA 2188150 A1 CA2188150 A1 CA 2188150A1 CA 002188150 A CA002188150 A CA 002188150A CA 2188150 A CA2188150 A CA 2188150A CA 2188150 A1 CA2188150 A1 CA 2188150A1
Authority
CA
Canada
Prior art keywords
disk
disk substrate
surface roughness
angstroms
substrate
Prior art date
Legal status (The legal status 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 status listed.)
Abandoned
Application number
CA002188150A
Other languages
French (fr)
Inventor
Oh-Hun Kwon
Current Assignee (The listed assignees may be inaccurate. Google has not performed a legal analysis and makes no representation or warranty as to the accuracy of the list.)
Saint Gobain Ceramics and Plastics Inc
Original Assignee
Individual
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 Individual filed Critical Individual
Publication of CA2188150A1 publication Critical patent/CA2188150A1/en
Abandoned legal-status Critical Current

Links

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
    • G11B5/84Processes or apparatus specially adapted for manufacturing record carriers
    • G11B5/8404Processes or apparatus specially adapted for manufacturing record carriers manufacturing base 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
    • G11B5/62Record 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
    • 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
    • G11B5/739Magnetic recording media substrates
    • G11B5/73911Inorganic substrates
    • GPHYSICS
    • G11INFORMATION STORAGE
    • G11BINFORMATION STORAGE BASED ON RELATIVE MOVEMENT BETWEEN RECORD CARRIER AND TRANSDUCER
    • G11B2220/00Record carriers by type
    • G11B2220/20Disc-shaped record carriers
    • YGENERAL TAGGING OF NEW TECHNOLOGICAL DEVELOPMENTS; GENERAL TAGGING OF CROSS-SECTIONAL TECHNOLOGIES SPANNING OVER SEVERAL SECTIONS OF THE IPC; TECHNICAL SUBJECTS COVERED BY FORMER USPC CROSS-REFERENCE ART COLLECTIONS [XRACs] AND DIGESTS
    • Y10TECHNICAL SUBJECTS COVERED BY FORMER USPC
    • Y10STECHNICAL SUBJECTS COVERED BY FORMER USPC CROSS-REFERENCE ART COLLECTIONS [XRACs] AND DIGESTS
    • Y10S428/00Stock material or miscellaneous articles
    • Y10S428/90Magnetic feature

Abstract

This invention relates to a disk substrate for use in a disk drive, the disk substrate consisting essentially of partially stabilized zirconia and having a surface roughness (Ra) of no more than 10 angstroms.

Description

NRC-3062 21881~ 0 Improved Disk Substrate Background of the Invention In the information systems presently used in computers and word processors, data (i.e., programs and files) are stored and retrieved through the disk drive.
The disk drive typically has three components: the read-write head ("head"), the actuator arm, and the hard magnetic disk ("disk"). Figure 1 discloses a conventional disk drive 1 in which the actuator arm 2 lQ moves the head 3 over disk 4 so that the circuitry on the head can magnetically transmit bits of information between leads (not shown) and the disk 4. Figure 2 discloses a conventional disk wherein a substrate 5 (typically an Al/Mg alloy) has deposited thereon, consecutively, an electroless or anodized coating (~i/P) 6, a magnetic coating 7, a protective overcoat 8, and a liquid lubricant 9.
Due to the high density of information typically stored on a disk, the head must come very close to the disk during data transmission in order to insure accurate transfer. Accordingly, the space between the head and the disk (called a "flying height" or "air gap") is often between about 100-150 nm (4-6 microinches). At such extremely small distances, both the head and the disk must be very flat. Thus, the material used for the disk ! should be very stiff and amenable to a fine finish.
When the disk and actuator arm move relative to each other, an air flow develops and allows the head to "float" above the disk. During operation, the head's ability to float prevents wear-inducing contact between the head and disk which degrades the accuracy of data transfer. However, the starting and stopping of the disk L - . ., . .. ... ~ . .. . . .. .

-or arm often produces physical co~tact between the head and disk. Therefore, it is also desirable to make the disk substrate from a material which is wear resistant.
As noted above, most conventional disks are made from a Mg/Al alloy overcoated with Ni/P and a magnetic film. This alloy has been selected as the material of choice for the disk due to its superior wear resistance, stiffness and polishablity, and performs well in the current relatively large disk drives.
However, increasing speed and capacity requirements are forcing disk drives to become smaller and smaller.
For example, the current hard disk is about 65-275 mm in diameter and 0.64 mm to 1.5 mm in thickness, and is expected to be less than about 38 mm in diameter and less than about 0.4 mm in thickness in the future. Likewise, the air gap will be reduced to no more than 50 nm (2 microinches). At these dimensions, it is believed that use of Al/Mg alloys as disk substrates will be problematic in that the elastic modulus of Al/Mg alloys (only about 80 GPa) will not provide the stiffness required in the thin disks of the future (wherein the required stiffness will likely be at least about 200 GPa).
Faced with this problem, the art has considered using alternative ceramics. It has been suggested that glass, glass ceramics, amorphous carbon, silicon, titanium, polymers, and stainless steels are the likely candidates for the next generation of disk substrates.
See B.Bhusan, "Magnetic Slider/Rigid Disk Substrate Materials and Disk Texturing Techniques-Status and Future Outlook", Advances in Information Storage Systems, Vol.
5, 1993, pp. 175-209. Moreover, Bhusan concludes thzt, of .. . , .. .. . .. .. , .. . , . . .. . . .. " .. .. .. .. ..... . .. . . . . . ...

this group, the most promising are glasses, glass ceramics and amorphous carbon because they possess adequate elastic modulus.
One other material which has been suggested for use S as a substrate for future disks is CV3 silicon carbide.
See Am. Cer. Soc. Bull. Vol. 72, No. 3 (March 1993),p.74.
However, CVD silicon carbide suffers from the disadvantages of high cost and directional (columnar) grain structure.
JP 62078716 discloses a zirconia based magnetic disk substrate for use in disk drives. However, the surface roughness (Ra) of this material is reported to be only 0.01 um (100 angstroms). JP 62078715 discloses a zirconia based magnetic disk substrate for use in disk drives.
However, the low density of this material would likely yield an even lower surface roughness (Ra).
EPO Patent Application 0 131 895 reports a zirconia based magnetic disk substrate for use in disk drives.
However, the best surface roughness (Ra) of any disclosed material is reported to be only 0.003 um (30 angstroms).
JP 01112518 discloses a zirconia based magnetic disk substrate for use in disk drives. However, the surface roughness (Ra) of this material is reported to be only 5-8 nm (50-80 angstroms).
Accordingly, there is a need for a disk drive material possessing superior wear resistance, stiffness and polishablity.

: - . -- -, -, =

NRC-3062 ~183150 Summary of the Invention In accordance with the present invention, there is provided a partially stabilized zirconia substrate (preferably in the form of a disk substrate for use in a disk drive), the substrate consisting essentially of partially stabilized zirconia and having a surface roughness (Ra) of no more than 1 nm (lO angstroms).
Also in accordance with the present invention, the-e is provided a disk substrate for use in a disk drive, the disk substrate consisting essentially of partial~y stabilized zirconia and having a textured surface.
Also in accordance with the present invention, there is provided a disk drive comprising: a) a head, and b) an underlying disk as disclosed above, wherein the in-use airgap between the head and the disk is no more than 50 nm (2 microinches).
Also in accordance with the present invention, there is provided a process comprising: a) polishing a partially stabilized zirconia substrate with a diamond or alumina paste to a finish of no more than 1 nm (10 angstroms).
Description of the Figures Figure 1 presents a conventional disk drive system.
Figure 2 presents a conventional disk.
Detailed Description of the Invention It is believed that the most of the promising disk substrate candidate materials poss~ss inadequate toughness or a too high surface roughness (Ra). In particular, they possess the following toughnesses:
Substrate Toughness (MPa m1~2) 1) glass 0.5 - 0.9 2) glass ceramics 2 3) amorphous carbon 4) silicon 2 5) CVD Silicon carbide 3 In contrast, it is believed that the toughness required for the thin disks of the future will be at least about 4 MPa ml/2 and the surface roughness (Ra) requirement will be no more than 1 nm (10 angstroms).
Without wishing to be tied to a theory, it is believed that high toughness is required in these future disk substrates because it affords superior machinability and damage tolerance, and the fine finish (low surface roughness) is required for increased recording density.
Because partially-stabilized zirconia typically has a toughness of at least about 7 MPa m1~2 and can now be made to have a surface roughness of no more than 1 nm (10 angstroms), it is believed that these materials will be required in the disks of the future.
For the purposes of this invention, "fracture toughness" is measured by the Chantikul indentation strength method as disclosed in the Journal of the American Ceramics Society, 64(9), 1981, pp. 539-44.
(CITE); surface roughness Ra" is the universally recognized as the arithmetic mean of the departures of the profile from the mean surface; and grit sizes used in finishing refer to the average diameter of the grit.
Any conventional partially-stabilized zirconia ~"PSZ") ceramic, such as yttria-partially stabilized tetragonal zirconia polycrystal ceramic ("YTZP"), may be used in accordance with the present invention.
Typically, commercial partially-stabilized zirconias have at least about 30% (and often more than about 70%) tetragonal zirconia and a toughness of at least about 4.5 MPa m"2, preferably at least about 6 MPa ml~2.
Preferably, the zirconia is partially stabilized by a - rare earth, and more preferably at a concentration of between about 2.5 mol% and about 6 mol~, as rare earth oxide, most preferably at a concentration of between about 2.5 mol% and about 4 mol%, as rare earth oxide.
In some embodiments, the zirconia is YZ110, an yttrium-stabilized zirconia available from the Norton Company of ~orcester, MA.
Any conventional method of making the zirconia disk substrate may be used. For example, in some embodiments, rare earth oxide powder and zirconia powder are mixed, the mixture is cipped (uniaxially or isostatically) at between 50 and 500 MPa to form a green piece; the green lS piece is sintered at between 1300C and 1500C for 0.5-4 hours to achieve a density of at least 95~i and the sintered piece is hipped in inert gas at between 1200C
and 1500C for between 0.5 and 4 hours to achieve a density of at least 99.9%.
Most preferably, yttria powder and zirconia powder are mixed, cold-pressed, sintered to at least 96~ density and hipped to at least 99.9% density.
In some embodiments, it is believed advantageous to have a highly pure disk substrate, that is, a substrate having less than 0.3% of impurity or sintering aid, especially if the impurity or sintering aid tends to form a second phase. Such typical sintering aids include silica, iron and manganese. It has been found that using YTZP powders, available from Daiichi Kigenso (DKK) of Osaka, Japan, without sintering aid produces a partially stabilized disk substrate having the desired levels of .. . . . .. ..

purity which can be finished to the desired levels of surface roughness (Ra). Accordingly, there is provided a partially stabilized zirconia disk substrate having no more than 0.3% impurity or sintering aid and a surface roughness of no more than 1 nm (10 angstroms).
In some preferred embodiments, it is believed advantageous to have no more than 0.1% porosity. It has been found that PSZ from commercially available DKK
powders provides a partially stabilized disk substrate having no more than 0.1% porosity which can be finished to the desired levels of surface roughness (Ra).
Disk preparation generally involves only two steps:
making a thin ceramic body and then finishing the body.
Any conventional method of making thin ceramic bodies may be used in accordance with the invention, including diamond saw slicing of ceramic rods, tape casting, extrusion, and die pressing. Preferably, the thin disk substrates are made by slicing a ceramic rod with a diamond saw. The slicing should produce a disk having an Ra of between about 2-7 um and a thickness of less than about 1 mm, preferably less than about 0.5 mm.
Any conventional lapping method may be used to help attain the required finish on the disk substrate of the present invention, including lapping with a diamond paste or alumina. The lapping should produce a finish of less than about 12.5 nm (125 angstroms). In preferred embodiments, the polishing entails selecting either a diamond paste or alumina grain having an average size of between about 3 and 15 um, preferably less than 10 um.
It has been found that polishing the lapped disk substrate with a fine diamond paste or alumina produces a finish of less than about 1 nm (10 angstroms). In . , . . .,, . , ... . - . . . - - . - . .

'~188 150 preferred embodiments, the polishing step uses diamond, alumina or a mixture thereof, having an average size of about 0.01 and 0.2 um, preferably less than 0.1 um.
Although a smooth disk surface is desirable for S accuracy, it is often the case that disk substrates which are too smooth stick to the head. Accordingly, disks often require a surface texture. Any conventional method of texturing may be used, including thermal etching, laser etching, chemical etching and plasma etching, and combinations thereof. If thermal etching is selected to texture zirconia, the temperature of the etch is typically between about 800 and 1400C, preferably about 1000C at about 30 minutes.
In other embodiments, zirconia toughened alumina may be used, preferably AZ67, available from the Norton Company of Worcester, MA. It is believed that lapplng and polishing commercial zirconia toughened alumina having a toughness of at least about 4.5 MPa m"2, preferably at least about 5 MPa ml~2 as described above yields the desired finish.
In still other embodiments, boron carbide may be selected. If boron carbide is selected as the disk substrate, any conventional boron carbide ceramic may be used. It is believed that when boron carbide is either hot pressed or sinter-hipped, and then lapped and polished as above yields the desired finish. It typically has a modulus of elasticity of at least about 435 GPa.
More preferably, the boron carbide also has a porosity of less than about 0.1% and a surface roughness (Ra) of no more than 1 nm (10 angstroms). In preferred embodiments, .. . . . . .. . . ... . . . . .. . . .. .

the boron carbide is Norbide, a hot-pressed boron carbide available from the Norton Company of Worcester, MA.
COMPARATIVE EXAMPLE
A YZ110-H blank rod having a 3.81 cm (1.5") diameter and a 7.62 cm ~3") length, available from the Norton Company of Worcester, MA, was sliced with a diamond saw.
The surface of this slice was subjected to a number of finishing steps including grinding, lapping and polishing steps.
In particular, the slice was first ground with a 320 grit diamond blank to produce a surface roughness (Ra) of about 0.110 um. Next, the lapped slice was serially lapped and polished with diamond on a 30.48 cm (12 inch) lapping machine according to the specifications set out in Table I below:
TABLE I

Slice Grit Size Wheel type Speed Pressure Duration Ra um rpm MPa (psi) min um - 20 A 40 alumina100 0.138 (20) 4 0.130 B 30 platen25 0.173 (25) 3 0.028 C 9 platen125 0.173 (25) 2 0.020 D 3 texmet200 0.207 (30) 1.2 0.012 E 1 cloth300 0.311 (45) 1.2 0.008 F 0.25 cloth400 0.414 (60) <1 0.005 This test slice did not achieve the desired 0.001 um ~10 angstrom) surface roughness (Ra).
EXAMPLE I
A YZl10-H blank rod having a 3.81 cm (1.5") diameter and a 7.62 cm (3") length, available from the Norton Company of Worcester, MA, was sliced with a diamond saw into six slices A to F.

.. . . . . . . . . . . . . . . . . . . . . .

Slices ~ and F were sliced at a higher feed rate. The thickest and thinnest cross sections, as well as the surface roughness Ra of these six slices are presented ln Table II. The surface roughness tRa) was measured by TENCOR.
TABLE II
Slice cm Thickest cm Thinnest Ra (um) A 0.1021 (0.0406 in) 0.1021 (0.0402 in) 2-7 B 0.1046 (0.0412 in) 0.1029 (0.0405 in) 2-7 C 0.1021 (0.0406 in) 0.1019 (0.0401 in) 2-7 D 0.0511 (0.0201 in) 0.0493 (0.0194 in) 2-6 E 0.0546 (0.0215 in) 0.0495 (0.0195 in) 2-7 F 0.0597 (0.0235 in) 0.0559 (0.0220 in) 2-5 ! These slices were subjected to standard lapping and polishing steps, and then final-polished with a 0.05 diamond paste to a surface roughness (Ra) of 1 nm (10 angstroms), as measured by TENCOR methodology. Lastly, one of the slices was textured by thermal etching at 1000C.
EXAMPLE II
Two Daiichi powders (3mol%Y-TZP and 4mol%Y-TZP) were cipped at 200 MPa to form green rods, sintered in alr at 1350 for 60 minutes to achieve at least 98% density, and hipped in argon at 1350C and 200 MPa for about ~5 minutes to produce rods having a density of at least 99.9~.
These dense rods were then sliced into disks of 25.4 mm diameter and 0.8 mm thickness. Final finish grinding of these slices was undertaken with #500 grit resin bonded diamond wheels.
The ground disk blanks were lapped using 9 um alumina grit on a cast-iron lapping wheel having slurry .. . . . . . . .

continuously dripping from the wheel. Lapping took about 30 minutes znd produced a surface roughness of about 12.5 nm (125 angstroms).
The lapped slices were then final-polished with a O.OS um alumina/diamond paste to a surface roughness (Ra~
of 1 nm (10 angstroms), as measured by TENCOR
methodology.
EXAMPLE III
This example proceed substantially similarly to Example II, except that the lapping step used 9 um alumina only and the final-polish step used 50 nm alumina only. The resulting disk substrate had a surface roughness of about 1 nm (10 angstroms), as measured by AFM.

Claims (8)

1. A disk substrate for use in a disk drive, the disk substrate selected from the group consisting of partially stabilized zirconia and zirconia toughened alumina, the disk substrate having a surface roughness (Ra) of no more than 1 nm (10 angstroms).
2. The disk substrate of claim 1 consisting essentially of partially stabilized zirconia comprising between about 2.5 mol% and about 6 mol% rare earth, as rare earth oxide.
3. The disk substrate of claim 2 having an impurity level of no more than 0.3%.
4. The disk substrate of claim 2 having a porosity of no more than 0.1%.
5. The disk substrate of claim 2 wherein the partially stabilized zirconia comprises about 4 mol% rare earth, as rare earth oxide.
6. A disk drive comprising:
a) a head, and b) a disk comprising the disk substrate of claim 1, wherein the airgap between the head and the disk is no more than 2 microinches.
7. A process comprising the steps of:
a) lapping a disk substrate selected from the group consisting of partially stabilized zirconia and zirconia toughened alumina with a diamond or alumina paste, or mixture thereof, having a grit size of between about 3 µm and 15 µm to a surface roughness (Ra) of about 50-125 angstroms, and b) polishing the disk substrate with a diamond or alumina paste, or mixture thereof, to a surface roughness (Ra) of no more than 10 angstroms.
8. A partially stabilized zirconia substrate consisting essentially of partially stabilized zirconia and having a surface roughness (Ra) of no more than 10 angstroms, the substrate produced by a process comprising the steps of:
a) lapping a disk substrate consisting essentially of partially stabilized zirconia with a diamond or alumina paste, or mixture thereof, having a grit size of between about 3 um and 15 um to a surface roughness (Ra) of about 125 angstroms, and b) polishing the disk substrate with a diamond or alumina paste, or mixture thereof, having an grit size of between 0.01 and 0.2 um to a surface roughness (Ra) of no more than 10 angstroms.
CA002188150A 1994-04-19 1995-04-18 Improved disk substrate Abandoned CA2188150A1 (en)

Applications Claiming Priority (2)

Application Number Priority Date Filing Date Title
US23004494A 1994-04-19 1994-04-19
US08/230,044 1994-04-19

Publications (1)

Publication Number Publication Date
CA2188150A1 true CA2188150A1 (en) 1995-10-26

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Country Status (6)

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EP (1) EP0756743A1 (en)
JP (1) JPH09512127A (en)
KR (1) KR970702550A (en)
CN (1) CN1147312A (en)
CA (1) CA2188150A1 (en)
WO (1) WO1995028703A1 (en)

Families Citing this family (3)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
JP3311308B2 (en) * 1998-03-03 2002-08-05 株式会社オハラ Glass ceramic substrate for perpendicular magnetic recording media
US6383645B1 (en) * 1998-03-23 2002-05-07 Kabushiki Kaisha Ohara Glass-ceramic substrate for an information storage medium
CN1151622C (en) * 2000-12-18 2004-05-26 信息产业部电信传输研究所 Pilot channel tracking method based on multipath channel energy window gravity center tracking loop

Family Cites Families (4)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
JPS6022733A (en) * 1983-07-19 1985-02-05 Hitachi Metals Ltd Substrate for magnetic disc
JPH0715753B2 (en) * 1985-08-22 1995-02-22 株式会社日立製作所 Magnetic recording medium
JPH0740350B2 (en) * 1985-09-30 1995-05-01 京セラ株式会社 Magnetic disk substrate
US4738885A (en) * 1986-02-24 1988-04-19 Kyocera Corporation Magnetic disk, substrate therefor and process for preparation thereof

Also Published As

Publication number Publication date
KR970702550A (en) 1997-05-13
JPH09512127A (en) 1997-12-02
EP0756743A1 (en) 1997-02-05
WO1995028703A1 (en) 1995-10-26
CN1147312A (en) 1997-04-09

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