CN102269926B - Method for optimizing optical proximity correction (OPC) of nonideal photoetching system based on Abbe vector imaging model - Google Patents

Method for optimizing optical proximity correction (OPC) of nonideal photoetching system based on Abbe vector imaging model Download PDF

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CN102269926B
CN102269926B CN2011102683288A CN201110268328A CN102269926B CN 102269926 B CN102269926 B CN 102269926B CN 2011102683288 A CN2011102683288 A CN 2011102683288A CN 201110268328 A CN201110268328 A CN 201110268328A CN 102269926 B CN102269926 B CN 102269926B
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马旭
李艳秋
董立松
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Beijing Institute of Technology BIT
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Abstract

The invention provides a method for optimizing optical proximity correction (OPC) of a nonideal photoetching system based on an Abbe vector imaging model. The method comprises the following steps of: setting transmittivity of an opening part and a light blocking part in a mask; setting a variable matrix Omega; setting a target function D as linear combination of an imaging evaluation function of an ideal image surface and an imaging evaluation function of an image surface of which the defocusing quantity is fnm; and guiding optimization on a mask pattern by using the variable matrix Omega and the target function D. By using the vector imaging model and taking vector characteristic of an electromagnetic field into consideration during acquisition of a space image, the optimized mask is suitable for the photoetching system with small numerical aperture (NA) and also suitable for the photoetching system of which the NA is more than 0.6. By the method, the gradient information of optimizing the target function is utilized and a steepest descent method is combined to optimize the pattern and the phase of an attenuated phase-shifting mask, so the optimization efficiency is high.

Description

Optimization method of non-ideal lithography system OPC based on Abbe vector imaging model
Technical Field
The invention relates to an optimization method of non-ideal lithography system OPC (lithography proximity correction) based on Abbe (Abbe) vector imaging model, belonging to the technical field of lithography resolution enhancement.
Background
Current large scale integrated circuits are commonly manufactured using photolithographic systems. The lithography system is mainly divided into: the device comprises an illumination system (comprising a light source and a condenser), a mask, a projection system and a wafer. Light rays emitted by the light source are focused by the condenser lens and then are incident to the mask, and the opening part of the mask is transparent; after passing through the mask, light is incident on the photoresist-coated wafer via the projection system, so that the mask pattern is reproduced on the wafer.
The mainstream lithography system at present is an ArF deep ultraviolet lithography system with the wavelength of 193nm, and as the node of the lithography technology enters 45nm-22nm, the key size of a circuit is far smaller than the wavelength of a light source. The interference and diffraction phenomena of the light are more pronounced, resulting in distortions and blurring of the lithographic image. For this reason, the lithography system must employ resolution enhancement techniques to improve the imaging quality. Optical proximity correction (optical proximity correction opc) is an important lithography resolution enhancement technique. OPC achieves the purpose of improving the photoetching imaging resolution by changing the mask pattern and adding a fine auxiliary pattern on the mask.
In order to further improve the imaging resolution of the lithography system, an immersion lithography system is commonly used in the industry. In the immersion lithography system, liquid with the refractive index larger than 1 is added between the lower surface of the last lens of the projection objective and a wafer, so that the aims of enlarging the numerical aperture (numerical aperture NA) and improving the imaging resolution are fulfilled. Since immersion lithography systems have the property of a high NA (NA > 1), scalar imaging models of lithography systems are no longer applicable when NA > 0.6. In order to obtain accurate imaging characteristics of an immersion lithography system, the mask in the immersion lithography system must be optimized using OPC techniques based on a vector imaging model.
In an actual lithography system, there are a number of process variations. On one hand, due to factors such as processing and adjustment, the projection system can generate certain influence on the phase of incident light, and further the imaging quality of the photoetching system is influenced, so that the photoetching system is a non-ideal photoetching system, and the influence is mainly reflected in two aspects of scalar aberration and polarization aberration of the projection system. On the other hand, due to the influence of factors such as control, the actual position of the wafer in the lithography system changes, and the actual image plane position (wafer position) deviates from the ideal image plane position of the lithography system, and this image plane deviation phenomenon appears as the image plane defocusing of the lithography system. The quality of an aerial image obtained at the actual image plane position differs greatly from that obtained at the ideal image plane. In order to design an OPC optimization scheme suitable for an actual lithography system, the influence of various process variations in the lithography system must be considered.
The related art (Journal of Optics, 2010, 12: 045601) proposes an OPC optimization method for enlarging the depth of focus of a lithography system based on a gradient for a partially coherent imaging system. However, the above method has the following two disadvantages: first, the above method is based on a scalar imaging model of the lithography system, and is therefore not suitable for high NA lithography systems. Second, the above method does not consider the influence of scalar aberration, polarization aberration, etc. of the lithography system, and is not suitable for a non-ideal lithography system.
Disclosure of Invention
The invention aims to provide an optimization method of non-ideal lithography system OPC based on an Abbe vector imaging model. The method adopts the OPC technology of a vector model to optimize the mask, and can be suitable for an immersion lithography system with high NA and a dry lithography system with low NA.
The technical scheme for realizing the invention is as follows:
an optimization method of non-ideal lithography system OPC based on Abbe vector imaging model comprises the following steps:
step 101, initializing the mask pattern M to a target pattern with size of NXN
102, setting the transmissivity of an opening part on the initial mask graph M to be 1 and the transmissivity of a light blocking area to be 0; setting a variable matrix Ω of N × N: when M (x, y) is 1,
Figure GDA0000158658760000031
when M (x, y) is 0,
Figure GDA0000158658760000032
wherein M (x, y) represents the transmittance of each pixel point on the mask pattern;
step 103, constructing the objective function D as an imaging evaluation function D at an ideal image surface1Image evaluation function D at image surface with defocus amount f2Linear combination of (i), i.e. D ═ η D1+(1-η)D2Wherein η ∈ (0, 1) is a weighting coefficient;
imaging evaluation function D1Set as the square of the Euler distance between the aerial image on the ideal image plane and the target pattern after amplitude modulation, i.e.
Figure GDA0000158658760000033
Wherein
Figure GDA0000158658760000034
Being a target patternPixel value, Inom(x, y) is the pixel value of a space image on an ideal image surface corresponding to the current mask, and omega epsilon (0, 1) is an amplitude modulation coefficient;
imaging evaluation function D2The defocus amount is set to be the square of the Euler distance between the aerial image on the f image plane and the target pattern after amplitude modulation, that is, the defocus amount is set to be the square of the Euler distance between the aerial image on the f image plane and the target pattern after amplitude modulation
Figure GDA0000158658760000035
Wherein Ioff(x, y) is the pixel value of the space image on the f image surface corresponding to the defocusing amount of the current mask;
step 104, calculating a gradient matrix of the objective function D to the variable matrix omega
Figure GDA0000158658760000036
Step 105, updating the variable matrix to be omega' by using the steepest descent method, namely
Figure GDA0000158658760000037
Wherein s is a preset optimization step length, and a mask graph corresponding to the current omega' is obtained
Figure GDA0000158658760000038
Figure GDA0000158658760000039
Step 106, calculating the current mask pattern
Figure GDA00001586587600000310
The corresponding objective function value D; when D is smaller than a preset threshold value or the number of times of updating the variable matrix omega reaches a preset upper limit value, the step 107 is entered, otherwise, the variable matrix omega is enabled to be omega', and the step 104 is returned;
step 107, terminating the optimization and intercepting the current mask pattern by using the square window
Figure GDA00001586587600000311
Central part of (2)
Figure GDA00001586587600000312
The side length of the square window is the smaller of the period of the target graph in the horizontal direction and the period of the target graph in the vertical direction;
step 108, for
Figure GDA00001586587600000313
Periodically extending in the horizontal direction and the vertical direction until the extended mask size is larger than or equal to the target pattern size, and obtaining the pattern
Figure GDA00001586587600000314
And determining the optimized mask pattern.
In step 103 of the present invention, the process of obtaining the aerial image on the ideal image plane corresponding to the current mask and the aerial image on the image plane with the defocus amount f corresponding to the current mask is as follows:
step 201, rasterizing a mask pattern M into N multiplied by N sub-regions;
step 202, grid the light source surface into a plurality of point light sources, and use the central point coordinates (x) of each grid areas,ys) Representing the point light source coordinates corresponding to the grid area;
step 203, acquiring the variation ξ of the phase of the incident light of the lithography system caused by δ according to the distance δ between the image plane where the space image needs to be acquired and the ideal image plane; wherein δ is 0 for the aerial image on the ideal image plane, and δ is f for the aerial image on the image plane with defocus amount f;
step 204, obtaining a scalar aberration matrix W (α ', β ') describing the scalar aberration of the projection system and a polarization aberration matrix J (α ', β ') describing the polarization aberration of the projection system, wherein (α ', β ', γ ') is a coordinate system of the global coordinate system on the image plane after Fourier transformation;
step 205, for a single point light source, utilize its coordinates (x)s,ys) The variation xi of the incident light phase, the scalar aberration matrix W (alpha ', beta') and the polarization aberration matrix J (alpha ', beta') are obtained, and when the point light source is illuminated, a space image I on an ideal image surface is obtainednoms,βs) And an aerial image I on the image surface with defocus foffs,βs);
Step 206, judging whether the space image I corresponding to all the point light sources is calculatednoms,βs) And Ioffs,βs) If yes, go to step 207, otherwise return to step 205;
step 207, according to the Abbe method, corresponding space image I to each point light sourcenoms,βs) Superposing to obtain a space image I on an ideal image surfacenomFor space image I corresponding to each point light sourceoffs,βs) Superposing to obtain a space image I on an image surface with a defocusing amount foff
In step 205, an aerial image I corresponding to the point light source is obtainednoms,βs) And Ioffs,βs) The specific process comprises the following steps:
setting a global coordinate system as follows: taking the direction of an optical axis as a z-axis, and establishing a global coordinate system (x, y, z) by the z-axis according to the principle of a left-hand coordinate system;
301, according to the coordinates (x) of the point light sources,ys) Calculating the near-field distribution E of the light waves emitted by the point light source passing through the NxN sub-regions on the mask; wherein E is an N × N vector matrix, each element of which is a 3 × 1 vector representing 3 components of the diffracted near-field distribution of the mask in the global coordinate system;
step 302, obtaining the electric field distribution of the light wave behind the entrance pupil of the projection system according to the near field distribution E
Figure GDA0000158658760000051
WhereinA vector matrix of N × N, each element of which is a 3 × 1 vector, representing 3 components of the electric field distribution behind the entrance pupil in the global coordinate system;
step 303, setting the propagation direction of the light wave in the projection system to be approximately parallel to the optical axis, and further according to the electric field distribution behind the entrance pupil
Figure GDA0000158658760000053
Scalar aberration matrix W (α ', β') and polarization aberration matrix J (α ', β') to obtain the electric field distribution of the light waves in front of the exit pupil of the projection system
Figure GDA0000158658760000054
Wherein the electric field distribution in front of the exit pupil
Figure GDA0000158658760000055
A vector matrix of N × N, each element of which is a 3 × 1 vector, representing 3 components of the electric field distribution in front of the exit pupil in the global coordinate system;
304, according to the electric field distribution in front of the exit pupil of the projection system
Figure GDA0000158658760000056
Obtaining electric field distribution behind the exit pupil of a projection system
Figure GDA0000158658760000057
305, utilizing the Walf Wolf optical imaging theory, according to the electric field distribution behind the exit pupilAnd the variation xi of the incident light phase to obtain the electric field distribution on the ideal image surface
Figure GDA0000158658760000059
And the electric field distribution on the image plane with defocus fAnd according to
Figure GDA00001586587600000511
Obtaining a space image I on an ideal image surface corresponding to a point light sourcenoms,βs) According toObtaining a spatial image I on an image surface with defocus f corresponding to a point light sourceoffs,βs)。
Advantageous effects
In the process of acquiring the space image of the lithography system, the influence of scalar aberration, polarization aberration and defocus of the non-ideal lithography system is considered, so that the optimization method can be suitable for the non-ideal lithography system.
Secondly, the vector imaging model utilized in the invention considers the vector characteristic of the electromagnetic field in the process of acquiring the space image, so that the optimized mask is not only suitable for a photoetching system with small NA, but also suitable for a photoetching system with NA more than 0.6.
Thirdly, the method optimizes the mask graph by utilizing the gradient information of the optimized objective function and combining the steepest descent method, and the optimization efficiency is high.
Drawings
FIG. 1 is a flowchart illustrating an OPC optimizing method for a non-ideal lithography system based on an Abbe vector imaging model according to the present invention.
FIG. 2 is a schematic diagram of a light wave emitted from a point light source passing through a mask and a projection system to form an aerial image at a wafer position.
FIG. 3 is a schematic diagram of wafer position deviation from an ideal image plane.
FIG. 4 is a schematic diagram of rasterizing a partially coherent light source plane in an embodiment of the present invention.
FIG. 5 is a schematic wavefront diagram of scalar aberrations and polarization aberrations (represented by Jones pupil) for a projection system of a particular lithography system.
FIG. 6 shows an initial mask and an optimized mask corresponding to dense lines under unpolarized illumination without aberrationMask center section cut with square window
Figure GDA0000158658760000062
And based on
Figure GDA0000158658760000063
Optimized mask after periodic continuation
Figure GDA0000158658760000064
Schematic representation of (a).
FIG. 7 is a diagram of an initial mask corresponding to dense lines and an optimized mask after periodic extension when there is no aberration under unpolarized illumination
Figure GDA0000158658760000065
Corresponding process window schematic.
FIG. 8 shows an initial mask and an optimized mask corresponding to dense lines when there is aberration under unpolarized illumination
Figure GDA0000158658760000066
Mask center section cut with square window
Figure GDA0000158658760000067
And based on
Figure GDA0000158658760000068
Optimized mask after periodic continuationSchematic representation of (a).
FIG. 9 is a diagram of an initial mask corresponding to dense lines and an optimized mask after periodic extension when there is aberration under unpolarized illumination
Figure GDA0000158658760000071
Corresponding process window schematic.
Detailed Description
The present invention will be further described in detail with reference to the accompanying drawings.
The principle of the invention is as follows: the process variation factors in an actual lithography system mainly include: exposure variation, defocus, scalar aberration, polarization aberration, and the like. The scalar aberration and the polarization aberration mainly affect the phase of the incident light of the projection system, and after the used lithography system is determined, the scalar aberration and the polarization aberration of the projection system can be obtained by using a ray tracing method. The stability of the lithography system to exposure variation and defocus can be evaluated using a process window. The horizontal axis of the process window is the defocus Depth (Depth of focus DOF), which represents the maximum difference between the actual wafer position and the ideal image plane on the premise that the imaging quality is acceptable. The vertical axis of the process window is Exposure depth (EL), which represents the acceptable Exposure variation range under the premise of acceptable imaging quality; EL is typically expressed as the amount of change in exposure as a percentage of the nominal exposure. The opening of the process window contains all the corresponding combinations of DOF and EL that meet the specific manufacturing process requirements. The specific manufacturing process requirements generally include Critical Dimension (CD) errors, sidewall angles of the imaged contours in the photoresist, and other parameters. When the process window opening corresponding to the photoetching system is large, the stability of the system to exposure variation and defocusing is high.
To expand the process window opening in the transverse axis (DOF) direction, i.e., to expand the gap between the actual wafer position and the ideal image plane, provided that the imaging quality is acceptable. The invention constructs a target function D as an imaging evaluation function D at an ideal image surface1Image evaluation function D at image surface with defocus amount f2Linear combination of (i), i.e. D ═ η D1+(1-η)D2Where η ∈ (0, 1) is a weighting coefficient.
In order to enlarge the process window opening in the direction of the longitudinal axis (EL), i.e. to enlarge the acceptable range of exposure variation, provided that the imaging quality is acceptable. The method of the invention should make the space image corresponding to the optimized OPC as close as possible to the target graph. The reason for this is that: when the aerial image is close to the target graph, the aerial image distribution has a relatively steep side wall angle, so that the relatively steep side wall angle of the imaging contour in the photoresist is favorably formed; meanwhile, the line width difference of the space image distributed on the cross sections with different heights is small, and the CD error caused by the change of the exposure can be reduced. Assuming that the size of the target pattern is NXN, the imaging evaluation function D of the invention1Set as the square of the Euler distance between the aerial image on the ideal image plane and the target pattern after amplitude modulation, i.e.
Figure GDA0000158658760000081
Wherein
Figure GDA0000158658760000082
Is the pixel value of the target pattern, InomAnd (x, y) is the pixel value of a space image on the ideal image surface corresponding to the current mask, and omega epsilon (0, 1) is an amplitude modulation coefficient. Imaging evaluation function D2The defocus amount is set to be the square of the Euler distance between the aerial image on the f image plane and the target pattern after amplitude modulation, that is, the defocus amount is set to be the square of the Euler distance between the aerial image on the f image plane and the target pattern after amplitude modulation
Figure GDA0000158658760000083
Wherein IoffAnd (x, y) is the pixel value of the space image on the image plane, which is the defocus amount corresponding to the current mask.
As shown in FIG. 1, the method for optimizing the OPC of the non-ideal lithography system based on the Abbe vector imaging model comprises the following specific steps:
step 101, initializing the mask pattern M to a target pattern with size of NXN
Figure GDA0000158658760000084
102, setting the transmissivity of an opening part on the initial mask graph M to be 1 and the transmissivity of a light blocking area to be 0; setting a variable matrix Ω of N × N: when M (x, y) is 1,
Figure GDA0000158658760000085
when M (x, y) is 0,
Figure GDA0000158658760000086
where M (x, y) represents the transmittance of each pixel on the mask pattern.
Step 103, constructing the objective function D as an imaging evaluation function D at an ideal image surface1Image evaluation function D at image surface with defocus amount f2Linear combination of (i), i.e. D ═ η D1+(1-η)D2Where η ∈ (0, 1) is a weighting coefficient.
Imaging evaluation function D1Set as the square of the Euler distance between the aerial image on the ideal image plane and the target pattern after amplitude modulation, i.e.
Figure GDA0000158658760000087
Wherein
Figure GDA0000158658760000088
Is the pixel value of the target pattern, InomAnd (x, y) is the pixel value of a space image on the ideal image surface corresponding to the current mask, and omega epsilon (0, 1) is an amplitude modulation coefficient.
Imaging evaluation function D2Set the defocus amount to be f space image on image surface and the amplitude modulatedSquares of Euler distances between target patterns, i.e.
Figure GDA0000158658760000091
Wherein IoffAnd (x, y) is the pixel value of the space image on the image plane, which is the defocus amount corresponding to the current mask.
In step 103 of the present invention, the process of obtaining the aerial image on the ideal image plane corresponding to the current mask and the aerial image on the image plane with the defocus amount f corresponding to the current mask is as follows:
variable predefinition
As shown in fig. 2, the direction of the optical axis is set as the z-axis, and a global coordinate system (x, y, z) is established with the z-axis according to the principle of the left-hand coordinate system. Let the global coordinate of any point light source on the partially coherent light source surface be (x)s,ys,zs) The cosine of the direction of the plane wave emitted from the point light source and incident on the mask is (alpha)s,βs,γs) Then the relationship between the global coordinate and the direction cosine is:
αs=xs·NAm,βs=ys·NAm <math> <mrow> <msub> <mi>&gamma;</mi> <mi>s</mi> </msub> <mo>=</mo> <mi>cos</mi> <mo>[</mo> <msup> <mi>sin</mi> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </msup> <mrow> <mo>(</mo> <msub> <mi>NA</mi> <mi>m</mi> </msub> <mo>&CenterDot;</mo> <msqrt> <msubsup> <mi>x</mi> <mi>s</mi> <mn>2</mn> </msubsup> <mo>+</mo> <msubsup> <mi>y</mi> <mi>s</mi> <mn>2</mn> </msubsup> </msqrt> <mo>)</mo> </mrow> <mo>]</mo> </mrow> </math>
wherein, NAmIs the projection system object-side numerical aperture.
Assuming that the global coordinate of any point on the mask is (x, y, z), the direction cosine of the plane wave incident from the mask to the projection system entrance pupil is (α, β, γ) based on the diffraction principle, where (α, β, γ) is the coordinate system after fourier transformation of the global coordinate system (x, y, z) on the mask (object plane).
Let the global coordinate of any point on the wafer (image plane) be (x)w,yw,zw) The direction cosine of the plane wave incident from the projection system exit pupil to the image plane is (α ', β', γ '), where (α', β ', γ') is the global coordinate system (x) on the wafer (image plane)w,yw,zw) And (4) carrying out a coordinate system after Fourier transformation.
Conversion relationship between global coordinate system and local coordinate system:
establishing a local coordinate system (e),eP),eThe axis being the direction of vibration of the TE-polarized light in the light emitted by the light source, ePThe axis is the vibration direction of the TM polarized light in the light emitted by the light source. Wave vector of
Figure GDA0000158658760000093
The plane formed by the wave vector and the optical axis is called the incident plane, the vibration direction of the TM polarized light is in the incident plane, and the vibration direction of the TE polarized light is perpendicular to the incident plane. The transformation relationship between the global coordinate system and the local coordinate system is:
<math> <mrow> <mfenced open='[' close=']'> <mtable> <mtr> <mtd> <msub> <mi>E</mi> <mi>x</mi> </msub> </mtd> </mtr> <mtr> <mtd> <msub> <mi>E</mi> <mi>y</mi> </msub> </mtd> </mtr> <mtr> <mtd> <msub> <mi>E</mi> <mi>z</mi> </msub> </mtd> </mtr> </mtable> </mfenced> <mo>=</mo> <mi>T</mi> <mo>&CenterDot;</mo> <mfenced open='[' close=']'> <mtable> <mtr> <mtd> <msub> <mi>E</mi> <mo>&perp;</mo> </msub> </mtd> </mtr> <mtr> <mtd> <msub> <mi>E</mi> <mi>P</mi> </msub> </mtd> </mtr> </mtable> </mfenced> </mrow> </math>
wherein E isx、EyAnd EzRespectively the component of the light wave electric field emitted by the light source in the global coordinate system, EAnd EPThe component of the light wave electric field emitted by the light source in the local coordinate system is as follows:
<math> <mrow> <mi>T</mi> <mo>=</mo> <mfenced open='[' close=']'> <mtable> <mtr> <mtd> <mo>-</mo> <mfrac> <mi>&beta;</mi> <mi>&rho;</mi> </mfrac> </mtd> <mtd> <mo>-</mo> <mfrac> <mi>&alpha;&gamma;</mi> <mi>&rho;</mi> </mfrac> </mtd> </mtr> <mtr> <mtd> <mfrac> <mi>&alpha;</mi> <mi>&rho;</mi> </mfrac> </mtd> <mtd> <mo>-</mo> <mfrac> <mi>&beta;&gamma;</mi> <mi>&rho;</mi> </mfrac> </mtd> </mtr> <mtr> <mtd> <mn>0</mn> </mtd> <mtd> <mi>&rho;</mi> </mtd> </mtr> </mtable> </mfenced> </mrow> </math>
wherein, <math> <mrow> <mi>&rho;</mi> <mo>=</mo> <msqrt> <msup> <mi>&alpha;</mi> <mn>2</mn> </msup> <mo>+</mo> <msup> <mi>&beta;</mi> <mn>2</mn> </msup> </msqrt> <mo>.</mo> </mrow> </math>
in an actual lithography system, there is a phenomenon in which the position of the wafer deviates from an ideal image plane, and the distance between the two is represented by δ. As shown in fig. 3. 301 is the distance from the actual position of the wafer to the ideal image plane, and its effect on the image is reflected in the change of the optical path length, as shown in 302, which can be obtained from the geometrical relationship:
Optical_pach=nwδ(1-cosθ)
wherein n iswTheta is the refractive index of the immersion liquid at the image side of the lithography system, and theta is the angle between the light ray and the optical axis.
The acquisition process of the aerial image is as follows:
step 201, the mask pattern M is rasterized into N × N sub-regions.
Step 202, grid the light source surface into a plurality of areas, each area is approximated by a point light source, and the center point coordinate (x) of each grid areas,ys) And representing the point light source coordinates corresponding to the grid area. As shown in fig. 4, the method of the present invention uses equally spaced lines parallel to the X-axis and Y-axis directions to grid the light source plane of a partially coherent light source into small squares of equal size.
Step 203, acquiring the variation ξ of the phase of the incident light of the lithography system caused by δ according to the distance δ between the image plane where the space image needs to be acquired and the ideal image plane; where δ is 0 for an aerial image on an ideal image plane, and δ is f for an aerial image on an image plane with defocus amount f.
Because the actual position of a wafer in the photoetching system changes under the influence of factors such as control and the like, the actual image plane position deviates from the position of an ideal image plane of the photoetching system, and defocusing amount is generated; the defocusing amount can bring the phase change of the incident light of the photoetching system, and the variable quantity xi is
<math> <mrow> <mi>&xi;</mi> <mo>=</mo> <msup> <mi>k</mi> <mo>&prime;</mo> </msup> <mo>&CenterDot;</mo> <msub> <mi>n</mi> <mi>w</mi> </msub> <mo>&CenterDot;</mo> <mi>&delta;</mi> <mo>&CenterDot;</mo> <mrow> <mo>(</mo> <mn>1</mn> <mo>-</mo> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> <mo>=</mo> <msup> <mi>k</mi> <mo>&prime;</mo> </msup> <mo>&CenterDot;</mo> <msub> <mi>n</mi> <mi>w</mi> </msub> <mo>&CenterDot;</mo> <mi>&delta;</mi> <mo>&CenterDot;</mo> <mrow> <mo>(</mo> <mn>1</mn> <mo>-</mo> <msqrt> <mn>1</mn> <mo>-</mo> <msup> <mi>&alpha;</mi> <mrow> <mo>&prime;</mo> <mn>2</mn> </mrow> </msup> <mo>-</mo> <msup> <mi>&beta;</mi> <mrow> <mo>&prime;</mo> <mn>2</mn> </mrow> </msup> </msqrt> <mo>)</mo> </mrow> <mo>,</mo> </mrow> </math>
Wherein <math> <mrow> <msup> <mi>k</mi> <mo>&prime;</mo> </msup> <mo>=</mo> <mfrac> <mrow> <mn>2</mn> <mi>&pi;</mi> <msub> <mi>n</mi> <mi>w</mi> </msub> </mrow> <mi>&lambda;</mi> </mfrac> </mrow> </math> Is the wave number.
When the space image on the ideal image surface is solved, delta is equal to 0, the solved defocusing amount is the space image on the f image surface, and delta is equal to f.
Step 204, obtaining a scalar aberration matrix W (α ', β ') and a polarization aberration matrix J (α ', β ') of the projection system, wherein (α ', β ', γ ') is a coordinate system of the global coordinate system on the image plane after fourier transformation.
The projection system is a non-ideal optical system due to processing, adjustment and other factors, and the phase of incident light is also affected to a certain extent. For low numerical aperture projection systems, only the scalar aberration matrix W (α ', β') is needed to describe the non-idealities of the projection system, assuming that the optical wavefront has the same amplitude over the entire pupil of the projection system. However, as the numerical aperture of the projection system increases, the vector imaging property of the light wave has a more significant effect on the aerial image at the wafer position, and therefore the present invention further considers the effect of the polarization aberration J (α ', β') on the aerial image at the wafer position.
The scalar aberration matrix W (α ', β') and the polarization aberration matrix J (α ', β') are each N × N matrices; each element in the W (α ', β') matrix is a numerical value that represents the number of wavelengths that the actual wave surface at the exit pupil differs from the ideal wave surface; j (α ', β') is an N × N vector matrix, each matrix element is a Jones matrix, and since TE and TM polarized light pass through the transformation matrix, both expressed in the form of xy components, the Jones matrix is specifically formed as:
<math> <mrow> <mi>J</mi> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> <mo>=</mo> <mfenced open='(' close=')'> <mtable> <mtr> <mtd> <msub> <mi>J</mi> <mi>xy</mi> </msub> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> </mtd> <mtd> <msub> <mi>J</mi> <mi>xy</mi> </msub> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> </mtd> </mtr> <mtr> <mtd> <msub> <mi>J</mi> <mi>yx</mi> </msub> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> </mtd> <mtd> <msub> <mi>J</mi> <mi>yy</mi> </msub> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> </mtd> </mtr> </mtable> </mfenced> </mrow> </math> m,n=1,2,...,N
Ji′,j' (α ', β ', m, n) (i ' ═ x, y; j ' ═ x, y) denotes the ratio of incident i ' polarized light to j ' polarized light after passing through the projection system.
Step 205, for a single point light source, utilize its coordinates (x)s,ys) The variation xi of the incident light phase, the scalar aberration matrix W (alpha ', beta') and the polarization aberration matrix J (alpha ', beta') are obtained, and when the point light source is illuminated, a space image I on an ideal image surface is obtainednoms,βs) And an aerial image I on the image surface with defocus foffs,βs)。
Step 206, judging whether the space image I corresponding to all the point light sources is calculatednoms,βs) And Ioffs,βs) If yes, go to step 207, otherwise return to step 205.
Step 207, according to the Abbe method, corresponding space image I to each point light sourcenoms,βs) Superposing to obtain a space image I on an ideal image surfacenomFor space image I corresponding to each point light sourceoffs,βs) Superposing to obtain a space image I on an image surface with a defocusing amount foff
In step 205, an aerial image I is obtainednoms,βs) And Ioffs,βs) The specific process comprises the following steps:
301, according to the coordinates (x) of the point light sources,ys) And calculating the near-field distribution E of the light wave emitted by the point light source passing through the N multiplied by N sub-regions on the mask.
Figure GDA0000158658760000121
Where E is an N × N vector matrix (if all elements of a matrix are matrices or vectors, it is called a vector matrix), and each element in the vector matrix is a 3 × 1 vector, which represents 3 components of the diffracted near-field distribution of the mask in the global coordinate system. e represents the multiplication of the corresponding elements of the two matrices.
Figure GDA0000158658760000122
Is an NxN vector matrix, and each element is an electric field vector of an electric field of the light wave emitted by the point light source in a global coordinate system; if the electric field of the light wave emitted by a point light source on the partially coherent light source is expressed as a local coordinate system
Figure GDA0000158658760000123
Figure GDA0000158658760000124
The electric field is then expressed in the global coordinate system as:
<math> <mrow> <msup> <msub> <mover> <mi>E</mi> <mi>u</mi> </mover> <mi>i</mi> </msub> <mo>&prime;</mo> </msup> <mo>=</mo> <mi>T</mi> <mo>&CenterDot;</mo> <msub> <mover> <mi>E</mi> <mi>u</mi> </mover> <mi>i</mi> </msub> </mrow> </math>
the diffraction matrix B of the mask is an N × N scalar matrix in which each element is a scalar, and according to the Hopkins (Hopkins) approximation, each element of B can be expressed as:
<math> <mrow> <mi>B</mi> <mrow> <mo>(</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> <mo>=</mo> <mi>exp</mi> <mrow> <mo>(</mo> <mfrac> <mrow> <mi>j</mi> <mn>2</mn> <mi>&pi;</mi> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> <mi>x</mi> </mrow> <mi>&lambda;</mi> </mfrac> <mo>)</mo> </mrow> <mi>exp</mi> <mrow> <mo>(</mo> <mfrac> <mrow> <mi>j</mi> <mn>2</mn> <mi>&pi;</mi> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <mi>y</mi> </mrow> <mi>&lambda;</mi> </mfrac> <mo>)</mo> </mrow> </mrow> </math>
<math> <mrow> <mo>=</mo> <mi>exp</mi> <mrow> <mo>(</mo> <mfrac> <mrow> <mi>j</mi> <mn>2</mn> <mi>&pi;</mi> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> <mi>m</mi> <mo>&times;</mo> <mi>pixel</mi> </mrow> <mi>&lambda;</mi> </mfrac> <mo>)</mo> </mrow> <mi>exp</mi> <mrow> <mo>(</mo> <mfrac> <mrow> <mi>j</mi> <mn>2</mn> <mi>&pi;</mi> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <mi>n</mi> <mo>&times;</mo> <mi>pixel</mi> </mrow> <mi>&lambda;</mi> </mfrac> <mo>)</mo> </mrow> <mo>,</mo> </mrow> </math> 1, 2, wherein pixel represents on the mask patternThe side length of each sub-region.
Step 302, obtaining the electric field distribution of the light wave behind the entrance pupil of the projection system according to the near field distribution E
<math> <mrow> <msubsup> <mi>E</mi> <mi>b</mi> <mi>ent</mi> </msubsup> <mrow> <mo>(</mo> <mi>&alpha;</mi> <mo>,</mo> <mi>&beta;</mi> <mo>)</mo> </mrow> <mo>.</mo> </mrow> </math>
The specific process of the step is as follows:
since each sub-region on the mask can be regarded as a secondary sub-light source, taking the center of the sub-region as the coordinate of the sub-region, according to the fourier optics theory, the electric field distribution in front of the projection system entrance pupil can be expressed as a function of α and β:
<math> <mrow> <msubsup> <mi>E</mi> <mi>l</mi> <mi>ent</mi> </msubsup> <mrow> <mo>(</mo> <mi>&alpha;</mi> <mo>,</mo> <mi>&beta;</mi> <mo>)</mo> </mrow> <mo>=</mo> <mfrac> <mi>&gamma;</mi> <mi>j&lambda;</mi> </mfrac> <mfrac> <msup> <mi>e</mi> <mrow> <mo>-</mo> <mi>jkr</mi> </mrow> </msup> <mi>r</mi> </mfrac> <mi>F</mi> <mo>{</mo> <mi>E</mi> <mo>}</mo> <mo>-</mo> <mo>-</mo> <mo>-</mo> <mrow> <mo>(</mo> <mn>3</mn> <mo>)</mo> </mrow> </mrow> </math>
wherein, because of the existence of N × N sub-regions on the mask, the electric field distribution in front of the entrance pupil
Figure GDA0000158658760000135
Vector of NxNA quantity matrix, each element of which is a 3 × 1 vector, representing 3 components of the electric field distribution in the global coordinate system in front of the entrance pupil. F { } denotes the fourier transform, r is the entrance pupil radius,
Figure GDA0000158658760000136
is the wave number, lambda is the wavelength of the light wave emitted by the point light source, nmIs the refractive index of the object space medium.
Since the reduction ratio of the projection system is larger, generally 4 times, the numerical aperture of the object space is smaller, which results in the electric field distribution in front of the entrance pupil
Figure GDA0000158658760000137
Is negligible, so that the electric field distribution in front of and behind the entrance pupil of the projection system is the same, i.e.
<math> <mrow> <msubsup> <mi>E</mi> <mi>b</mi> <mi>ent</mi> </msubsup> <mrow> <mo>(</mo> <mi>&alpha;</mi> <mo>,</mo> <mi>&beta;</mi> <mo>)</mo> </mrow> <mo>=</mo> <msubsup> <mi>E</mi> <mi>l</mi> <mi>ent</mi> </msubsup> <mrow> <mo>(</mo> <mi>&alpha;</mi> <mo>,</mo> <mi>&beta;</mi> <mo>)</mo> </mrow> <mo>=</mo> <mfrac> <mi>&gamma;</mi> <mi>j&lambda;</mi> </mfrac> <mfrac> <msup> <mi>e</mi> <mrow> <mo>-</mo> <mi>jkr</mi> </mrow> </msup> <mi>r</mi> </mfrac> <mi>F</mi> <mo>{</mo> <mi>E</mi> <mo>}</mo> <mo>-</mo> <mo>-</mo> <mo>-</mo> <mrow> <mo>(</mo> <mn>4</mn> <mo>)</mo> </mrow> </mrow> </math>
Wherein, because of the existence of N × N sub-regions on the mask, the electric field distribution behind the entrance pupil
Figure GDA0000158658760000139
Is an N × N vector matrix, each element of which is a 3 × 1 vector representing 3 components of the electric field distribution behind the entrance pupil in the global coordinate system.
Step 303, setting the propagation direction of the light wave in the projection system to be approximately parallel to the optical axis, and further according to the electric field distribution behind the entrance pupil
Figure GDA0000158658760000141
Scalar aberration matrix W (α ', β') and polarization aberration matrix J (α ', β') to obtain the electric field distribution of the light waves in front of the exit pupil of the projection system
Figure GDA0000158658760000142
The specific process of the step is as follows:
for an ideal projection system without aberrations, the mapping process of the electric field distribution behind the entrance pupil and in front of the exit pupil can be expressed in the form of a product of a low pass filter function and a correction factor, i.e.:
<math> <mrow> <msubsup> <mover> <mi>E</mi> <mo>^</mo> </mover> <mi>l</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> <mo>=</mo> <mi>cUe</mi> <msubsup> <mi>E</mi> <mi>b</mi> <mi>ent</mi> </msubsup> <mrow> <mo>(</mo> <mi>&alpha;</mi> <mo>,</mo> <mi>&beta;</mi> <mo>)</mo> </mrow> </mrow> </math>
wherein the electric field distribution in front of the exit pupilAn N × N vector matrix, each element of which is a 3 × 1 vector representing 3 components of the electric field distribution in front of the exit pupil in the global coordinate system; c is a constant correction factor and the low-pass filter function U is an N × N scalar matrix representing the finite acceptance of the diffraction spectrum by the numerical aperture of the projection system, i.e. the value inside the pupil is 1 and the value outside the pupil is 0, as follows:
<math> <mrow> <mi>U</mi> <mo>=</mo> <mfenced open='{' close=''> <mtable> <mtr> <mtd> <mn>1</mn> </mtd> <mtd> <msqrt> <msup> <mi>f</mi> <mn>2</mn> </msup> <mo>+</mo> <msup> <mi>g</mi> <mn>2</mn> </msup> </msqrt> <mo>&le;</mo> <mn>1</mn> </mtd> </mtr> <mtr> <mtd> <mn>0</mn> </mtd> <mtd> <mi>elsewhere</mi> </mtd> </mtr> </mtable> </mfenced> </mrow> </math>
where (f, g) is the normalized global coordinate on the entrance pupil.
The constant correction factor c can be expressed as:
<math> <mrow> <mi>c</mi> <mo>=</mo> <mfrac> <mi>r</mi> <msup> <mi>r</mi> <mo>&prime;</mo> </msup> </mfrac> <msqrt> <mfrac> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> <mi>&gamma;</mi> </mfrac> </msqrt> <mfrac> <msub> <mi>n</mi> <mi>w</mi> </msub> <mi>R</mi> </mfrac> </mrow> </math>
where r and r' are the projection system entrance and exit pupil radii, respectively, nwR is the demagnification of an ideal projection system, typically 4, for the refractive index of the immersion liquid at the image side of the lithography system.
Since the propagation direction of the light waves between the entrance and exit pupils of the projection system is approximately parallel to the optical axis, the phase difference between the back of the entrance pupil and the front of the exit pupil is the same for any of (α ', β'). Since it is ultimately required to solve the aerial image (i.e., the light intensity distribution) on the wafer, the constant phase difference between the back of the entrance pupil and the front of the exit pupil is negligible. The electric field distribution in front of the exit pupil can thus be found to be:
<math> <mrow> <msubsup> <mover> <mi>E</mi> <mo>^</mo> </mover> <mi>l</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> <mo>=</mo> <mfrac> <mn>1</mn> <msup> <mi>&lambda;r</mi> <mo>&prime;</mo> </msup> </mfrac> <msqrt> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> <mi>&gamma;</mi> </msqrt> <mfrac> <msub> <mi>n</mi> <mi>w</mi> </msub> <mi>R</mi> </mfrac> <mi>UeF</mi> <mo>{</mo> <mi>E</mi> <mo>}</mo> </mrow> </math>
because the projection system is a non-ideal optical system caused by factors such as processing and adjustment, the electric field distribution in front of the exit pupil of the non-ideal lithography system is obtained according to the electric field distribution in front of the exit pupil of the ideal lithography system by considering the influence of scalar aberration W (alpha ', beta') and polarization aberration J (alpha ', beta'),
<math> <mrow> <msubsup> <mi>E</mi> <mi>l</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> <mo>=</mo> <mfrac> <mn>1</mn> <msup> <mi>&lambda;r</mi> <mo>&prime;</mo> </msup> </mfrac> <msqrt> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> <mi>&gamma;</mi> </msqrt> <mfrac> <msub> <mi>n</mi> <mi>w</mi> </msub> <mi>R</mi> </mfrac> <mi>UeJ</mi> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> <mi>eF</mi> <mo>{</mo> <mi>E</mi> <mo>}</mo> <msup> <mi>ee</mi> <mrow> <mi>j</mi> <mn>2</mn> <mi>&pi;W</mi> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> </mrow> </msup> <mo>-</mo> <mo>-</mo> <mo>-</mo> <mrow> <mo>(</mo> <mn>5</mn> <mo>)</mo> </mrow> </mrow> </math>
304, according to the electric field distribution in front of the exit pupil of the projection system
Figure GDA0000158658760000152
Obtaining electric field distribution behind the exit pupil of a projection system
Figure GDA0000158658760000153
According to the rotation effect of the TM component of the electromagnetic field between the front and the back of the exit pupil, the electric field in the global coordinate system at the front and the back of the exit pupil is expressed as: vector matrix of NxN
Figure GDA0000158658760000154
And
Figure GDA0000158658760000155
Figure GDA0000158658760000156
and
Figure GDA0000158658760000157
each element of (a) is as follows:
<math> <mrow> <msubsup> <mi>E</mi> <mi>l</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> <mo>=</mo> <msup> <mrow> <mo></mo> <mo>[</mo> <msubsup> <mi>E</mi> <mi>lx</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> <mo>;</mo> <msubsup> <mi>E</mi> <mi>ly</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> <mo>;</mo> <msubsup> <mi>E</mi> <mi>lz</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> <mo>]</mo> <mo></mo> </mrow> <mi>T</mi> </msup> </mrow> </math>
<math> <mrow> <msubsup> <mi>E</mi> <mi>b</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> <mo>=</mo> <msup> <mrow> <mo></mo> <mo>[</mo> <msubsup> <mi>E</mi> <mi>bx</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> <mo>;</mo> <msubsup> <mi>E</mi> <mi>by</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> <mo>;</mo> <msubsup> <mi>E</mi> <mi>b</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> <mo>]</mo> <mo></mo> </mrow> <mi>T</mi> </msup> </mrow> </math>
where m, N is 1, 2, as, N, α ═ cos Φ ' sin θ ', β ═ sin Φ ' sin θ ', γ ═ cos θ ', that is, the direction cosine (wave vector) of the plane wave incident on the image plane from the projection system exit pupil is set to be equal toPhi 'and theta' are the azimuth and elevation angles, respectively, of the wave vector
Figure GDA00001586587600001511
And
Figure GDA00001586587600001512
the relation of (A) is as follows:
<math> <mrow> <msubsup> <mi>E</mi> <mi>b</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> <mo>=</mo> <mi>Ve</mi> <msubsup> <mi>E</mi> <mi>l</mi> <mi>ext</mi> </msubsup> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> <mo>-</mo> <mo>-</mo> <mo>-</mo> <mrow> <mo>(</mo> <mn>6</mn> <mo>)</mo> </mrow> </mrow> </math>
where V is an N × N vector matrix, and each element is a 3 × 3 matrix:
<math> <mrow> <mi>V</mi> <mrow> <mo>(</mo> <mi>m</mi> <mo>,</mo> <mi>n</mi> <mo>)</mo> </mrow> <mo>=</mo> <mfenced open='[' close=']'> <mtable> <mtr> <mtd> <msup> <mrow> <mi>cos</mi> <mi>&phi;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <msup> <mrow> <mo>-</mo> <mi>sin</mi> <mi>&phi;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <mn>0</mn> </mtd> </mtr> <mtr> <mtd> <msup> <mrow> <mi>sin</mi> <mi>&phi;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <msup> <mrow> <mi>cos</mi> <mi>&phi;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <mn>0</mn> </mtd> </mtr> <mtr> <mtd> <mn>0</mn> </mtd> <mtd> <mn>0</mn> </mtd> <mtd> <mn>1</mn> </mtd> </mtr> </mtable> </mfenced> <mo>&CenterDot;</mo> <mfenced open='[' close=']'> <mtable> <mtr> <mtd> <msup> <mrow> <mi>cos</mi> <mi>&theta;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <mn>0</mn> </mtd> <mtd> <msup> <mrow> <mi>sin</mi> <mi>&theta;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> </mtr> <mtr> <mtd> <mn>0</mn> </mtd> <mtd> <mn>0</mn> </mtd> <mtd> <mn>1</mn> </mtd> </mtr> <mtr> <mtd> <msup> <mrow> <mo>-</mo> <mi>sin</mi> <mi>&theta;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <mn>0</mn> </mtd> <mtd> <msup> <mrow> <mi>cos</mi> <mi>&theta;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> </mtr> </mtable> </mfenced> <mo>&CenterDot;</mo> <mfenced open='[' close=']'> <mtable> <mtr> <mtd> <msup> <mrow> <mi>cos</mi> <mi>&phi;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <msup> <mrow> <mi>sin</mi> <mi>&phi;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <mn>0</mn> </mtd> </mtr> <mtr> <mtd> <msup> <mrow> <mo>-</mo> <mi>sin</mi> <mi>&phi;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <msup> <mrow> <mi>cos</mi> <mi>&phi;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <mn>0</mn> </mtd> </mtr> <mtr> <mtd> <mn>0</mn> </mtd> <mtd> <mn>0</mn> </mtd> <mtd> <mn>1</mn> </mtd> </mtr> </mtable> </mfenced> </mrow> </math>
<math> <mrow> <mo>=</mo> <mfenced open='[' close=']'> <mtable> <mtr> <mtd> <msup> <mi>cos</mi> <mn>2</mn> </msup> <msup> <mi>&phi;</mi> <mo>&prime;</mo> </msup> <msup> <mrow> <mi>cos</mi> <mi>&theta;</mi> </mrow> <mo>&prime;</mo> </msup> <mo>+</mo> <msup> <mi>sin</mi> <mn>2</mn> </msup> <msup> <mi>&phi;</mi> <mo>&prime;</mo> </msup> </mtd> <mtd> <mi>cos</mi> <msup> <mi>&phi;</mi> <mo>&prime;</mo> </msup> <mi>sin</mi> <msup> <mi>&phi;</mi> <mo>&prime;</mo> </msup> <mrow> <mo>(</mo> <mi>cos</mi> <msup> <mi>&theta;</mi> <mo>&prime;</mo> </msup> <mo>-</mo> <mn>1</mn> <mo>)</mo> </mrow> </mtd> <mtd> <mi>cos</mi> <msup> <mi>&phi;</mi> <mo>&prime;</mo> </msup> <mi>sin</mi> <msup> <mi>&theta;</mi> <mo>&prime;</mo> </msup> </mtd> </mtr> <mtr> <mtd> <mi>cos</mi> <msup> <mi>&phi;</mi> <mo>&prime;</mo> </msup> <mi>sin</mi> <msup> <mi>&phi;</mi> <mo>&prime;</mo> </msup> <mrow> <mo>(</mo> <msup> <mrow> <mi>cos</mi> <mi>&theta;</mi> </mrow> <mo>&prime;</mo> </msup> <mo>-</mo> <mn>1</mn> <mo>)</mo> </mrow> </mtd> <mtd> <msup> <mi>sin</mi> <mn>2</mn> </msup> <msup> <mi>&phi;</mi> <mo>&prime;</mo> </msup> <mi>cos</mi> <msup> <mi>&theta;</mi> <mo>&prime;</mo> </msup> <mo>+</mo> <msup> <mi>cos</mi> <mn>2</mn> </msup> <msup> <mi>&phi;</mi> <mo>&prime;</mo> </msup> </mtd> <mtd> <mi>sin</mi> <msup> <mi>&phi;</mi> <mo>&prime;</mo> </msup> <mi>sin</mi> <msup> <mi>&theta;</mi> <mo>&prime;</mo> </msup> </mtd> </mtr> <mtr> <mtd> <msup> <mrow> <mo>-</mo> <mi>cos</mi> <mi>&phi;</mi> </mrow> <mo>&prime;</mo> </msup> <msup> <mrow> <mi>sin</mi> <mi>&theta;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <mo>-</mo> <msup> <mrow> <mi>sin</mi> <mi>&phi;</mi> </mrow> <mo>&prime;</mo> </msup> <mi>sin</mi> <msup> <mi>&theta;</mi> <mo>&prime;</mo> </msup> </mtd> <mtd> <mi>cos</mi> <msup> <mi>&theta;</mi> <mo>&prime;</mo> </msup> </mtd> </mtr> </mtable> </mfenced> </mrow> </math>
<math> <mrow> <mo>=</mo> <mfenced open='[' close=']'> <mtable> <mtr> <mtd> <mfrac> <mrow> <msup> <mi>&beta;</mi> <mrow> <mo>&prime;</mo> <mn>2</mn> </mrow> </msup> <mo>+</mo> <msup> <mi>&alpha;</mi> <mrow> <mo>&prime;</mo> <mn>2</mn> </mrow> </msup> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> </mrow> <mrow> <mn>1</mn> <mo>-</mo> <msup> <mi>&gamma;</mi> <mrow> <mo>&prime;</mo> <mn>2</mn> </mrow> </msup> </mrow> </mfrac> </mtd> <mtd> <mo>-</mo> <mfrac> <mrow> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> </mrow> <mrow> <mn>1</mn> <mo>+</mo> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> </mrow> </mfrac> </mtd> <mtd> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> </mtd> </mtr> <mtr> <mtd> <mo>-</mo> <mfrac> <mrow> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> </mrow> <mrow> <mn>1</mn> <mo>+</mo> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> </mrow> </mfrac> </mtd> <mtd> <mfrac> <mrow> <msup> <mi>&alpha;</mi> <mrow> <mo>&prime;</mo> <mn>2</mn> </mrow> </msup> <mo>+</mo> <msup> <mi>&beta;</mi> <mrow> <mo>&prime;</mo> <mn>2</mn> </mrow> </msup> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> </mrow> <mrow> <mn>1</mn> <mo>-</mo> <msup> <mi>&gamma;</mi> <mrow> <mo>&prime;</mo> <mn>2</mn> </mrow> </msup> </mrow> </mfrac> </mtd> <mtd> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> </mtd> </mtr> <mtr> <mtd> <msup> <mrow> <mo>-</mo> <mi>&alpha;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <msup> <mrow> <mo>-</mo> <mi>&beta;</mi> </mrow> <mo>&prime;</mo> </msup> </mtd> <mtd> <msub> <mi>&gamma;</mi> <mo>&prime;</mo> </msub> </mtd> </mtr> </mtable> </mfenced> </mrow> </math> m,n=1,2,...,N
step 305, utilize WoThe theory of optical imaging of the Lev Wolf is based on the electric field distribution behind the exit pupilObtaining electric field distribution on ideal image surface
Figure GDA0000158658760000162
And according toObtaining space image I of point light source corresponding to ideal image surfacenoms,βs)。
According to the electric field distribution behind the exit pupil by using Walf Wolf optical imaging theory
Figure GDA0000158658760000164
And the variation xi of the incident light phase, and acquiring the defocusing amount as the electric field distribution on the f image surface
Figure GDA0000158658760000165
And according to
Figure GDA0000158658760000166
Obtaining a space image I on an image surface with f defocusing amount corresponding to a point light sourceoffs,βs)。
The specific process of the step is as follows:
when the variation ξ of the phase of the incident light of the lithography system caused by the defocus δ of the non-ideal lithography system is not considered, the electric field distribution at the wafer position is shown as the formula (7):
<math> <mrow> <msup> <mover> <mi>E</mi> <mo>^</mo> </mover> <mi>wafer</mi> </msup> <mo>=</mo> <mfrac> <mrow> <mn>2</mn> <mi>&pi;&lambda;</mi> <msup> <mi>r</mi> <mo>&prime;</mo> </msup> </mrow> <msubsup> <mi>jn</mi> <mi>w</mi> <mn>2</mn> </msubsup> </mfrac> <msup> <mi>e</mi> <mrow> <mi>j</mi> <msup> <mi>k</mi> <mo>&prime;</mo> </msup> <msup> <mi>r</mi> <mo>&prime;</mo> </msup> <msup> <mi>F</mi> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </msup> </mrow> </msup> <mo>{</mo> <mfrac> <mn>1</mn> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> </mfrac> <msubsup> <mi>E</mi> <mi>b</mi> <mi>ext</mi> </msubsup> <mo>}</mo> <mo>-</mo> <mo>-</mo> <mo>-</mo> <mrow> <mo>(</mo> <mn>7</mn> <mo>)</mo> </mrow> </mrow> </math>
wherein,f-1{ } is an inverse Fourier transform. Substituting equations (5) and (6) into equation (7) and ignoring the constant phase term, we can:
<math> <mrow> <msup> <mover> <mi>E</mi> <mo>^</mo> </mover> <mi>wafer</mi> </msup> <mo>=</mo> <mfrac> <mrow> <mn>2</mn> <mi>&pi;</mi> </mrow> <mrow> <msub> <mi>n</mi> <mi>w</mi> </msub> <mi>R</mi> </mrow> </mfrac> <msup> <mi>F</mi> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </msup> <mo>{</mo> <msqrt> <mfrac> <mi>&gamma;</mi> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> </mfrac> </msqrt> <mi>eVeUe J</mi> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> <mi>eF</mi> <mo>{</mo> <mi>E</mi> <mo>}</mo> <mi>e</mi> <msup> <mi>e</mi> <mrow> <mi>j</mi> <mn>2</mn> <mi>&pi;W</mi> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> </mrow> </msup> <mo>}</mo> <mo>-</mo> <mo>-</mo> <mo>-</mo> <mrow> <mo>(</mo> <mn>8</mn> <mo>)</mo> </mrow> </mrow> </math>
for a non-ideal lithography system, when there is a distance δ between the image plane of the computed aerial image and the ideal image plane, it is necessary to consider the influence of the δ -induced phase change ξ of the incident light of the lithography system.
The electric field distribution on the non-ideal lithography system is then:
<math> <mrow> <msup> <mi>E</mi> <mi>wafer</mi> </msup> <mo>=</mo> <mfrac> <mrow> <mn>2</mn> <mi>&pi;&lambda;</mi> <msup> <mi>r</mi> <mo>&prime;</mo> </msup> </mrow> <msubsup> <mi>jn</mi> <mi>w</mi> <mn>2</mn> </msubsup> </mfrac> <msup> <mi>e</mi> <mrow> <mi>j</mi> <msup> <mi>k</mi> <mo>&prime;</mo> </msup> <msup> <mi>r</mi> <mo>&prime;</mo> </msup> </mrow> </msup> <msup> <mi>F</mi> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </msup> <mo>{</mo> <mfrac> <msup> <mi>e</mi> <mi>j&xi;</mi> </msup> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> </mfrac> <mi>e</mi> <msubsup> <mi>E</mi> <mi>b</mi> <mi>ext</mi> </msubsup> <mo>}</mo> <mo>-</mo> <mo>-</mo> <mo>-</mo> <mrow> <mo>(</mo> <mn>9</mn> <mo>)</mo> </mrow> </mrow> </math>
let δ be f, then
Figure GDA00001586587600001611
The defocus amount is the electric field distribution on the f image plane.
Let δ equal 0, then The electric field distribution on the ideal image surface.
When the formulas (1), (5) and (6) are substituted into the formula (9), a point light source (. alpha.) can be obtaineds,βs) The light intensity distribution of the image plane when illuminated, namely:
<math> <mrow> <msup> <mi>E</mi> <mi>wafer</mi> </msup> <mrow> <mo>(</mo> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <mo>,</mo> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> <mo>)</mo> </mrow> <mo>=</mo> <mfrac> <mrow> <mn>2</mn> <mi>&pi;</mi> </mrow> <mrow> <msub> <mi>n</mi> <mi>w</mi> </msub> <mi>R</mi> </mrow> </mfrac> <msup> <mi>F</mi> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </msup> <mo>{</mo> <msqrt> <mfrac> <mi>&gamma;</mi> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> </mfrac> </msqrt> <mi>e</mi> <msup> <mi>e</mi> <mi>j&xi;</mi> </msup> <mi>eVeUeJ</mi> <mrow> <mo>(</mo> <mrow> <mo></mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> </mrow> <mo>)</mo> </mrow> <mi>eF</mi> <mo>{</mo> <msub> <mi>E</mi> <mi>i</mi> </msub> <mmultiscripts> <mi>e</mi> <mo>&prime;</mo> </mmultiscripts> <mi>BeM</mi> <mo>}</mo> <mi>e</mi> <msup> <mi>e</mi> <mrow> <mi>j</mi> <mn>2</mn> <mi>&pi;W</mi> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> </mrow> </msup> <mo>}</mo> <mo>-</mo> <mo>-</mo> <mo>-</mo> <mrow> <mo>(</mo> <mn>10</mn> <mo>)</mo> </mrow> </mrow> </math>
due to Ei' the value of the middle element is independent of the mask coordinates, so the above equation can be written as:
<math> <mrow> <msup> <mi>E</mi> <mi>wafer</mi> </msup> <mrow> <mo>(</mo> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <mo>,</mo> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> <mo>)</mo> </mrow> <mo>=</mo> <mfrac> <mrow> <mn>2</mn> <mi>&pi;</mi> </mrow> <msub> <mi>nw</mi> <mi>R</mi> </msub> </mfrac> <msup> <mi>F</mi> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </msup> <mo>{</mo> <msup> <mi>V</mi> <mo>&prime;</mo> </msup> <mo>}</mo> <mo>&CircleTimes;</mo> <mrow> <mo>(</mo> <mi>BeM</mi> <mo>)</mo> </mrow> </mrow> </math>
wherein
Figure GDA0000158658760000173
Which represents a convolution of the signals of the first and second, <math> <mrow> <msup> <mi>V</mi> <mo>&prime;</mo> </msup> <mo>=</mo> <msqrt> <mfrac> <mi>&gamma;</mi> <msup> <mi>&gamma;</mi> <mo>&prime;</mo> </msup> </mfrac> </msqrt> <mi>e</mi> <msup> <mi>e</mi> <mrow> <mi>j&xi;</mi> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> </mrow> </msup> <mi>eVeUeJ</mi> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> <mi>e</mi> <msub> <mi>E</mi> <mi>i</mi> </msub> <mmultiscripts> <mi>e</mi> <mo>&prime;</mo> </mmultiscripts> <msup> <mi>e</mi> <mrow> <mi>j</mi> <mn>2</mn> <mi>&pi;W</mi> <mrow> <mo>(</mo> <msup> <mi>&alpha;</mi> <mo>&prime;</mo> </msup> <mo>,</mo> <msup> <mi>&beta;</mi> <mo>&prime;</mo> </msup> <mo>)</mo> </mrow> </mrow> </msup> </mrow> </math> is an N × N vector matrix, each matrix element is a 3 × 1 vector (v)x′,vy′,vz′)TWherein v isx′,vy′,vz' is a function of both alpha ' and beta '.
Then Ewafers,βs) The three components in the global coordinate system are
<math> <mrow> <msubsup> <mi>E</mi> <mi>P</mi> <mi>wafer</mi> </msubsup> <mrow> <mo>(</mo> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <mo>,</mo> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> <mo>)</mo> </mrow> <mo>=</mo> <msub> <mi>H</mi> <mi>p</mi> </msub> <mo>&CircleTimes;</mo> <mrow> <mo>(</mo> <mi>BeM</mi> <mo>)</mo> </mrow> </mrow> </math>
Wherein,
Figure GDA0000158658760000176
p is x, y, z, where Vp 'is an N × N scalar matrix composed of x components of elements of the vector matrix V'.
<math> <mrow> <mi>I</mi> <mrow> <mo>(</mo> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <mo>,</mo> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> <mo>)</mo> </mrow> <mo>=</mo> <munder> <mi>&Sigma;</mi> <mrow> <mi>p</mi> <mo>=</mo> <mi>x</mi> <mo>,</mo> <mi>y</mi> <mo>,</mo> <mi>x</mi> </mrow> </munder> <msubsup> <mrow> <mo>|</mo> <mo>|</mo> <msub> <mi>H</mi> <mi>p</mi> </msub> <mo>&CircleTimes;</mo> <mrow> <mo>(</mo> <mi>BeM</mi> <mo>)</mo> </mrow> <mo>|</mo> <mo>|</mo> </mrow> <mn>2</mn> <mn>2</mn> </msubsup> </mrow> </math>
Wherein
Figure GDA0000158658760000178
Representing the matrix modulo and squared. Wherein HpAnd B are both (. alpha.)s,βs) Are respectively marked as
Figure GDA0000158658760000179
And
Figure GDA00001586587600001710
thus the above formula can be written as:
<math> <mrow> <mi>I</mi> <mrow> <mo>(</mo> <msub> <mtext>&alpha;</mtext> <mi>s</mi> </msub> <mo>,</mo> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> <mo>)</mo> </mrow> <mo>=</mo> <munder> <mi>&Sigma;</mi> <mrow> <mi>p</mi> <mo>=</mo> <mi>x</mi> <mo>,</mo> <mi>y</mi> <mo>,</mo> <mi>x</mi> </mrow> </munder> <msubsup> <mrow> <mo>|</mo> <mo>|</mo> <msubsup> <mi>H</mi> <mi>p</mi> <mrow> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> </mrow> </msubsup> <mo>&CircleTimes;</mo> <mrow> <mo>(</mo> <msup> <mi>B</mi> <mrow> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> </mrow> </msup> <mi>eM</mi> <mo>)</mo> </mrow> <mo>|</mo> <mo>|</mo> </mrow> <mn>2</mn> <mn>2</mn> </msubsup> </mrow> </math>
order to
Figure GDA00001586587600001712
If the coefficient δ is f, then Ioffs,βs)=I(αs,βs) (ii) a Order to
Figure GDA00001586587600001713
When the coefficient δ is 0, then Inoms,βs)=I(αs,βs)。
The space image I on the ideal image surface corresponding to the point light source is obtained by the above formulanoms,βs) And a space image I on an image surface with defocusing amount f corresponding to the point light sourceoffs,βs) (ii) a According to the Abbe principle, then in step 207, the space image I on the ideal image surface under the illumination of the partial coherent light sourcenomAnd an aerial image I on the image plane with defocus foffCan be expressed as:
order to
Figure GDA00001586587600001714
When the coefficient δ is 0, then <math> <mrow> <msub> <mi>I</mi> <mi>nom</mi> </msub> <mo>=</mo> <mi>I</mi> <mo>=</mo> <mfrac> <mn>1</mn> <msub> <mi>N</mi> <mi>s</mi> </msub> </mfrac> <munder> <mi>&Sigma;</mi> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> </munder> <munder> <mi>&Sigma;</mi> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> </munder> <munder> <mi>&Sigma;</mi> <mrow> <mi>p</mi> <mo>=</mo> <mi>x</mi> <mo>,</mo> <mi>y</mi> <mo>,</mo> <mi>z</mi> </mrow> </munder> <msubsup> <mrow> <mo>|</mo> <mo>|</mo> <msubsup> <mi>H</mi> <mi>p</mi> <mrow> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> </mrow> </msubsup> <mo>&CircleTimes;</mo> <mrow> <mo>(</mo> <msup> <mi>B</mi> <mrow> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> </mrow> </msup> <mi>eM</mi> <mo>)</mo> </mrow> <mo>|</mo> <mo>|</mo> </mrow> <mn>2</mn> <mn>2</mn> </msubsup> </mrow> </math>
Order to
Figure GDA0000158658760000181
If the coefficient δ is f, then <math> <mrow> <msub> <mi>I</mi> <mi>off</mi> </msub> <mo>=</mo> <mi>I</mi> <mo>=</mo> <mfrac> <mn>1</mn> <msub> <mi>N</mi> <mi>s</mi> </msub> </mfrac> <munder> <mi>&Sigma;</mi> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> </munder> <munder> <mi>&Sigma;</mi> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> </munder> <munder> <mi>&Sigma;</mi> <mrow> <mi>p</mi> <mo>=</mo> <mi>x</mi> <mo>,</mo> <mi>y</mi> <mo>,</mo> <mi>z</mi> </mrow> </munder> <msubsup> <mrow> <mo>|</mo> <mo>|</mo> <msubsup> <mi>H</mi> <mi>p</mi> <mrow> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> </mrow> </msubsup> <mo>&CircleTimes;</mo> <mrow> <mo>(</mo> <msup> <mi>B</mi> <mrow> <msub> <mi>&alpha;</mi> <mi>s</mi> </msub> <msub> <mi>&beta;</mi> <mi>s</mi> </msub> </mrow> </msup> <mi>eM</mi> <mo>)</mo> </mrow> <mo>|</mo> <mo>|</mo> </mrow> <mn>2</mn> <mn>2</mn> </msubsup> </mrow> </math>
Wherein N issIs the number of sampling points of the partially coherent light source. If TE polarized illumination is used, equation (2) is set as:
Figure GDA0000158658760000183
the obtained aerial image at the wafer position is I ═ ITE. If TM polarized illumination is used, equation (2) is set as:
Figure GDA0000158658760000184
the obtained aerial image at the wafer position is I ═ ITM. If unpolarized illumination is used, the aerial image at the wafer location is
Figure GDA0000158658760000185
Step 104, calculating a gradient matrix of the objective function D to the variable matrix omega
Figure GDA0000158658760000186
In the invention, the gradient matrix of the objective function D to the variable matrix omega
Figure GDA0000158658760000187
Can be calculated as:
<math> <mrow> <mo>&dtri;</mo> <mi>D</mi> <mo>=</mo> <msub> <mrow> <mo>&dtri;</mo> <mi>D</mi> </mrow> <mn>1</mn> </msub> <mo>+</mo> <msub> <mrow> <mo>&dtri;</mo> <mi>D</mi> </mrow> <mn>2</mn> </msub> <mo>-</mo> <mo>-</mo> <mo>-</mo> <mrow> <mo>(</mo> <mn>11</mn> <mo>)</mo> </mrow> </mrow> </math>
wherein,
Figure GDA0000158658760000189
(12)
Figure GDA00001586587600001810
wherein,*to express a conjugate fortuneCalculating;οindicating that the matrix is rotated 180 degrees in both the transverse and longitudinal directions.
Figure GDA00001586587600001811
The expression (2) can be set as follows:
Figure GDA00001586587600001812
and (6) derivation and calculation.The expression (2) can be set as follows:
Figure GDA00001586587600001814
and (6) derivation and calculation. When TE polarized illumination is used, ρTE=2,ρ TM0; when TM polarized illumination is used, ρTE=0,ρ TM2; when unpolarized illumination is used, ρTE=1,ρTM1. Is calculated by the formula (12)
Figure GDA00001586587600001815
In this case, δ in equation (9) is set to 0, and the gradient of the imaging evaluation function corresponding to the ideal image plane is calculated. (11) In the formula
Figure GDA00001586587600001816
The formula (2) is the same as the formula (12), but δ in the formula (9) is set to f, so that the gradient of the imaging evaluation function at the image plane corresponding to the defocus amount f is calculated.
Step 105, updating the variable matrix to be omega' by using the steepest descent method, namely
Figure GDA00001586587600001817
s is a preset optimization step length. Further obtaining the mask pattern corresponding to the current omega
Figure GDA00001586587600001819
In the course of the OPC optimization process,
Figure GDA00001586587600001820
has a value range of
Figure GDA00001586587600001821
The value range of omega (x, y) is omega (x, y) epsilon [ - ∞, + ∞]。
Step 106, calculating the current mask pattern
Figure GDA0000158658760000191
The corresponding objective function value D; and when the D is smaller than a preset threshold value or the number of times of updating the variable matrix omega reaches a preset upper limit value, the step 107 is entered, otherwise, the variable matrix omega is enabled to be omega', and the step 104 is returned.
Step 107, terminating the optimization, and intercepting the current mask pattern by using a square window
Figure GDA0000158658760000192
Central part of (2)
Figure GDA0000158658760000193
The side length of the square window is the smaller of the period of the target graph in the horizontal direction and the period of the target graph in the vertical direction.
Step 108, pair
Figure GDA0000158658760000194
Periodically extending in the horizontal direction and the vertical direction until the extended mask size is larger than or equal to the target pattern size, and obtaining the pattern
Figure GDA0000158658760000195
And determining the optimized mask pattern.
Example of implementation of the invention:
as shown in FIG. 5, the projection system using the laboratory design in the simulation is viewed off-axisThe aberration at the field points is obtained by ray tracing (since in the field of numerical computation a two-dimensional graph is essentially a matrix-here, in effect, a two-dimensional wave surface map is drawn corresponding to a scalar aberration matrix, with the values at each coordinate point on the map corresponding one-to-one to the values of the elements of the matrix). 501 is a diagram of the aberration of the field point scale, and 502-509 are 8 Jones pupil components of the polarization aberration of the field point. 502. 503 are each JxxReal and imaginary parts of (c). 504. 505 are respectively JxyReal and imaginary parts of (c). 506. 507 are respectively JyxReal and imaginary parts of (c). 508. 509 are each JyyReal and imaginary parts of (c).
As shown in FIG. 6, when there is no aberration under unpolarized illumination, the initial mask and the optimized mask corresponding to dense lines
Figure GDA0000158658760000196
Mask center section cut with square window
Figure GDA0000158658760000197
And based on
Figure GDA0000158658760000198
Optimized mask after periodic continuation
Figure GDA0000158658760000199
Schematic representation of (a). 601 is an initial binary mask diagram with a critical dimension of 90nm, white for clear areas with a refractive index of 1, and gray for block areas with a refractive index of 0. The mask pattern lies in the XY plane with the lines parallel to the Y axis. 602 is the mask pattern optimized by the method of the present invention 603 denotes the central part of the mask, cut with a square window
Figure GDA00001586587600001911
Figure GDA00001586587600001911
604 are based onOptimized mask after periodic continuation
Figure GDA00001586587600001913
FIG. 7 is a diagram of an initial mask corresponding to dense lines and an optimized mask after periodic extension when there is no aberration under unpolarized illumination
Figure GDA0000158658760000201
Corresponding process window schematic. 701 is a process window corresponding to the initial mask, and 702 is an optimized mask after periodic continuation
Figure GDA0000158658760000202
Corresponding process window.
As shown in FIG. 8, when there is aberration under unpolarized illumination, the initial mask and the optimized mask corresponding to dense lines
Figure GDA0000158658760000203
Mask center section cut with square window
Figure GDA0000158658760000204
And based on
Figure GDA0000158658760000205
Optimized mask after periodic continuation
Figure GDA0000158658760000206
Schematic representation of (a). 801 is an initial binary mask diagram with a critical dimension of 90nm, white for clear areas with a refractive index of 1 and gray for block areas with a refractive index of 0. The mask pattern lies in the XY plane with the lines parallel to the Y axis. 802 is the mask pattern optimized by the method of the present invention
Figure GDA0000158658760000207
803 denotes the central part of the mask, cut with a square window
Figure GDA0000158658760000208
804 are based on
Figure GDA0000158658760000209
Optimized mask after periodic continuation
Figure GDA00001586587600002010
FIG. 9 is a diagram of an initial mask corresponding to dense lines and an optimized mask after periodic extension when there is aberration under unpolarized illumination
Figure GDA00001586587600002011
Corresponding process window schematic. 901 is the process window corresponding to the initial mask, 902 is the optimized mask after periodic continuationCorresponding process window.
Comparing 701, 702, 901 and 902, it can be known that the method of the present invention can effectively enlarge the process window under the condition of aberration and no aberration, that is, effectively improve the stability of the lithography system to the process variation factors such as exposure variation, defocus, scalar aberration and polarization aberration.
Although the embodiments of the present invention have been described in conjunction with the accompanying drawings, it will be understood that many variations, substitutions and modifications may be made by those skilled in the art without departing from the principles of the invention and these are intended to be within the scope of the invention.

Claims (3)

1. An OPC optimization method based on an Abbe vector imaging model non-ideal lithography system is characterized by comprising the following specific steps:
step 101, initializing the mask pattern M to a target pattern with size of NXN
Figure FDA0000158658750000011
102, setting the transmissivity of an opening part on the initial mask graph M to be 1 and the transmissivity of a light blocking area to be 0; setting a variable matrix Ω of N × N: when M (x, y) ═ MWhen the pressure of the mixture is 1, the pressure is lower,
Figure FDA0000158658750000012
when M (x, y) is 0,
Figure FDA0000158658750000013
wherein M (x, y) represents the transmittance of each pixel point on the mask pattern;
step 103, constructing the objective function D as an imaging evaluation function D at an ideal image surface1Image evaluation function D at image surface with defocus amount f2Linear combination of (i), i.e. D ═ η D1+(1-η)D2Wherein, eta belongs to (0, 1) as a weighting coefficient;
imaging evaluation function D1Set as the square of the Euler distance between the aerial image on the ideal image plane and the target pattern after amplitude modulation, i.e.
Figure FDA0000158658750000014
Wherein
Figure FDA0000158658750000015
Is the pixel value of the target pattern, Inom(x, y) is the pixel value of a space image on an ideal image surface corresponding to the current mask, and omega epsilon (0, 1) is an amplitude modulation coefficient;
imaging evaluation function D2The defocus amount is set to be the square of the Euler distance between the aerial image on the f image plane and the target pattern after amplitude modulation, that is, the defocus amount is set to be the square of the Euler distance between the aerial image on the f image plane and the target pattern after amplitude modulation
Figure FDA0000158658750000016
Wherein Ioff(x, y) is the pixel value of the space image on the f image surface corresponding to the defocusing amount of the current mask;
the process for acquiring the space image on the image surface of the projection objective corresponding to the current mask and the space image on the image surface with the defocus amount f corresponding to the current mask is as follows:
step 201, rasterizing a mask pattern M into N multiplied by N sub-regions;
step 202, grid the light source surface into a plurality of point light sources,using the center point coordinates (x) of each grid areas,ys) Representing the point light source coordinates corresponding to the grid area;
step 203, acquiring the variation ξ of the phase of the incident light of the lithography system caused by δ according to the distance δ between the image plane where the space image needs to be acquired and the ideal image plane; wherein δ is 0 for the aerial image on the ideal image plane, and δ is f for the aerial image on the image plane with defocus amount f;
step 204, obtaining a scalar aberration matrix W (α ', β ') describing the scalar aberration of the projection system and a polarization aberration matrix J (α ', β ') describing the polarization aberration of the projection system, wherein (α ', β ', γ ') is a coordinate system of the global coordinate system on the image plane after Fourier transformation;
step 205, for a single point light source, utilize its coordinates (x)s,ys) The variation xi of the incident light phase, the scalar aberration matrix W (alpha ', beta') and the polarization aberration matrix J (alpha ', beta') are obtained, and when the point light source is illuminated, a space image I on an ideal image surface is obtainednoms,βs) And an aerial image I on the image surface with defocus foffs,βs);
Step 206, judging whether the space image I corresponding to all the point light sources is calculatednoms,βs) And Ioffs,βs) If yes, go to step 207, otherwise return to step 205;
step 207, according to the Abbe method, corresponding space image I to each point light sourcenoms,βs) Superposing to obtain a space image I on an ideal image surfacenomFor space image I corresponding to each point light sourceoffs,βs) Superposing to obtain a space image I on an image surface with a defocusing amount foff
Step 104, calculating a gradient matrix of the objective function D to the variable matrix omega
Figure FDA0000158658750000021
Step 105, using the steepest descent methodUpdating the variable matrix to omega', i.e.
Figure FDA0000158658750000022
Wherein s is a preset optimization step length, and a mask graph corresponding to the current omega' is obtained
Figure FDA0000158658750000023
Figure FDA0000158658750000024
Step 106, calculating the current mask pattern
Figure FDA0000158658750000025
The corresponding objective function value D; when D is smaller than a preset threshold value or the number of times of updating the variable matrix omega reaches a preset upper limit value, the step 107 is entered, otherwise, the variable matrix omega is enabled to be omega', and the step 104 is returned;
step 107, terminating the optimization and intercepting the current mask pattern by using the square window
Figure FDA0000158658750000026
Central part of (2)
Figure FDA0000158658750000027
The side length of the square window is the smaller of the period of the target graph in the horizontal direction and the period of the target graph in the vertical direction;
step 108, for
Figure FDA0000158658750000028
Periodically extending in the horizontal direction and the vertical direction until the extended mask size is larger than or equal to the target pattern size, and obtaining the pattern
Figure FDA0000158658750000029
And determining the optimized mask pattern.
2. The optimization method of claim 1, wherein in the step 205, an aerial image I corresponding to the point light source is obtainednoms,βs) And Ioffs,βs) The specific process comprises the following steps:
setting a global coordinate system as follows: taking the direction of an optical axis as a z-axis, and establishing a global coordinate system (x, y, z) by the z-axis according to the principle of a left-hand coordinate system;
301, according to the coordinates (x) of the point light sources,ys) Calculating the near-field distribution E of the light waves emitted by the point light source passing through the NxN sub-regions on the mask; wherein E is an N × N vector matrix, each element of which is a 3 × 1 vector representing 3 components of the diffracted near-field distribution of the mask in the global coordinate system;
step 302, obtaining the electric field distribution of the light wave behind the entrance pupil of the projection system according to the near field distribution E
Figure FDA0000158658750000031
Wherein
Figure FDA0000158658750000032
A vector matrix of N × N, each element of which is a 3 × 1 vector, representing 3 components of the electric field distribution behind the entrance pupil in the global coordinate system;
step 303, setting the propagation direction of the light wave in the projection system to be approximately parallel to the optical axis, and further according to the electric field distribution behind the entrance pupil
Figure FDA0000158658750000033
Scalar aberration matrix W (α ', β') and polarization aberration matrix J (α ', β') to obtain the electric field distribution of the light waves in front of the exit pupil of the projection system
Figure FDA0000158658750000034
Wherein the electric field distribution in front of the exit pupil
Figure FDA0000158658750000035
Vector moment of NxNAn array, each element of which is a 3 x 1 vector, representing 3 components of the electric field distribution in the global coordinate system in front of the exit pupil;
304, according to the electric field distribution in front of the exit pupil of the projection system
Figure FDA0000158658750000036
Obtaining electric field distribution behind the exit pupil of a projection system
Figure FDA0000158658750000037
305, utilizing the Walf Wolf optical imaging theory, according to the electric field distribution behind the exit pupil
Figure FDA0000158658750000038
And the variation xi of the incident light phase to obtain the electric field distribution on the ideal image surface
Figure FDA0000158658750000039
And the electric field distribution on the image plane with defocus f
Figure FDA00001586587500000310
And according to
Figure FDA00001586587500000311
Obtaining a space image I on an ideal image surface corresponding to a point light sourcenoms,βs) According to
Figure FDA00001586587500000312
Obtaining a spatial image I on an image surface with defocus f corresponding to a point light sourceoffs,βs)。
3. The optimization method of claim 1, wherein the step 202 of rasterizing the light source area into a plurality of point light sources is: the light source surface of the partially coherent light source is rasterized into small squares of equal size with equally spaced lines parallel to the X-axis and Y-axis directions.
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