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Fast 3D thick mask model for full-chip EUVL simulations

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<strong>Fast</strong> <strong>3D</strong> <strong>thick</strong> <strong>mask</strong> <strong>model</strong> <strong>for</strong> <strong>full</strong>-<strong>chip</strong> <strong>EUVL</strong> <strong>simulations</strong><br />

Peng Liu*, Xiaobo Xie, Wei Liu, Keith Gronlund<br />

ASML Brion Technologies, 4211 Burton Drive, Santa Clara, CA, USA 95054<br />

ABSTRACT<br />

Extreme ultraviolet lithography (<strong>EUVL</strong>) uses a 13.5nm exposure wavelength, all-reflective projection optics, and a<br />

reflective <strong>mask</strong> under an oblique illumination with a chief ray angle of about 6 degrees to print device patterns. This<br />

imaging configuration leads to many challenges related to <strong>3D</strong> <strong>mask</strong> topography. In order to accurately predict and<br />

correct these problems, it is important to use a <strong>3D</strong> <strong>mask</strong> <strong>model</strong> in <strong>full</strong>-<strong>chip</strong> <strong>EUVL</strong> applications such as optical proximity<br />

correction (OPC) and verifications. In this work, a fast approximate <strong>3D</strong> <strong>mask</strong> <strong>model</strong> developed previously <strong>for</strong> <strong>full</strong>-<strong>chip</strong><br />

deep ultraviolet (DUV) applications is extended and greatly enhanced <strong>for</strong> EUV applications and its accuracy is evaluated<br />

against a rigorous <strong>3D</strong> <strong>mask</strong> <strong>model</strong>.<br />

Keywords: EUV, <strong>3D</strong> <strong>mask</strong>, best focus shift, pattern shift, shadowing effect<br />

1. INTRODUCTION<br />

Extreme ultraviolet lithography (<strong>EUVL</strong>) is a promising technology <strong>for</strong> 1x node and below logic and memory device<br />

patterning. It uses a 13.5nm exposure wavelength, all-reflective projection optics, and a reflective <strong>mask</strong> under an oblique<br />

illumination with a chief ray angle of about 6 degrees. While these reflective imaging conditions are required because<br />

conventional optical materials are highly absorptive at the EUV wavelength, they also cause many undesired effects<br />

related to <strong>3D</strong> <strong>mask</strong> topography. Even though <strong>EUVL</strong> uses a much shorter wavelength to image relatively large feature<br />

sizes (as compared to the wavelength) than deep ultraviolet (DUV) lithography, it actually has more <strong>3D</strong> <strong>mask</strong><br />

topography related challenges, which include pattern-dependent best focus shift, pattern shift, and shadowing effect.<br />

Pattern-dependent best focus shift is not unique to EUV lithography. It has been observed in DUV lithography in many<br />

cases already 1-3 . The root cause can be traced to the <strong>3D</strong> <strong>mask</strong> topography induced phase distortions in the transmitted<br />

field of a DUV <strong>mask</strong> 3 . Similarly, the <strong>3D</strong> topography of an EUV <strong>mask</strong> can also introduce pattern-dependent phase<br />

distortions in the reflected field, resulting in best focus variations among different device features on the wafer and<br />

there<strong>for</strong>e degradation in the common process window. Other effects are more unique to EUV lithography as they<br />

originate from the reflective imaging configuration of the oblique chief ray angle in conjunction with the <strong>3D</strong> <strong>mask</strong><br />

topography. This configuration leads to a generally asymmetric illumination seen by the <strong>mask</strong> and, there<strong>for</strong>e, some<br />

<strong>EUVL</strong>-specific printing effects which are not seen or can be avoided in the imaging configuration of DUV lithography.<br />

One of such effects is asymmetric shadowing effect that presents itself as HV print bias between horizontal (H) and<br />

vertical (V) features. Although it can be <strong>model</strong>ed to a certain degree using the rule-based HV <strong>mask</strong> bias in the thin <strong>mask</strong><br />

<strong>model</strong> 4 , the accuracy becomes inadequate as the feature size reduces 5 . Pattern shift is another such effect caused by<br />

<strong>mask</strong>-side non-telecentricity due to the oblique chief ray angle. It is important to note that the large global pattern shift<br />

observed in early EUV <strong>simulations</strong> using <strong>3D</strong> <strong>mask</strong> <strong>model</strong>s is largely a <strong>model</strong>ing artifact and can be corrected by<br />

trans<strong>for</strong>ming the <strong>mask</strong> diffraction coefficient to the optimum object plane be<strong>for</strong>e passing it to the subsequent simulation<br />

steps 4-5 . This process mimics the EUV scanner setup stage that moves the <strong>mask</strong> to the optimum <strong>mask</strong> focal plane.<br />

However there still exists a residual, pattern-dependent pattern shift caused by the <strong>3D</strong> <strong>mask</strong> topography even after the<br />

<strong>mask</strong> is placed at the optimum <strong>mask</strong> focal plane. There<strong>for</strong>e <strong>3D</strong> <strong>mask</strong> topography plays an important role in many of the<br />

challenges in EUV lithography. In order to accurately predict and correct these problems, it is important to use a <strong>3D</strong><br />

<strong>mask</strong> <strong>model</strong> in <strong>full</strong>-<strong>chip</strong> <strong>EUVL</strong> applications such as optical proximity correction (OPC) and verifications.<br />

Although rigorous <strong>3D</strong> <strong>mask</strong> <strong>model</strong>s based on methods such as finite difference time domain (FDTD) 6 and rigorous<br />

coupled wave analysis (RCWA) 7 are available, they are computationally too expensive <strong>for</strong> large area or <strong>full</strong>-<strong>chip</strong><br />

applications. In this work, a fast approximate <strong>3D</strong> <strong>mask</strong> <strong>model</strong> developed previously <strong>for</strong> <strong>full</strong>-<strong>chip</strong> DUV applications is<br />

extended and greatly enhanced <strong>for</strong> EUV applications, and its accuracy is evaluated against a rigorous <strong>3D</strong> <strong>mask</strong> <strong>model</strong>.<br />

*peng.liu@asml.com, 1-408-200-0843<br />

Extreme Ultraviolet (EUV) Lithography IV, edited by Patrick P. Naulleau, Proc. of SPIE Vol. 8679, 86790W<br />

© 2013 SPIE · CCC code: 0277-786X/13/$18 · doi: 10.1117/12.2010818<br />

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In the following sections, we first discuss some special considerations in <strong>EUVL</strong> <strong>simulations</strong> with rigorous <strong>3D</strong> <strong>mask</strong><br />

<strong>model</strong>s. These considerations are required in order to obtain realistic simulation results. Then we describe the<br />

development of the fast <strong>3D</strong> <strong>mask</strong> <strong>model</strong> <strong>for</strong> <strong>full</strong>-<strong>chip</strong> EUV applications, followed by simulation case studies to validate<br />

its accuracy against a rigorous <strong>3D</strong> <strong>mask</strong> <strong>model</strong>. A summary of this work is given in the end.<br />

2. <strong>EUVL</strong> SIMULATION CONSIDERATIONS<br />

Due to limited availability of experimental data <strong>for</strong> future device dimensions, the rigorous simulation remains the main<br />

vehicle to study the various effects in EUV lithography. In this work rigorous <strong>simulations</strong> will be used to generate<br />

reference data to evaluate the accuracy of the fast <strong>3D</strong> <strong>mask</strong> <strong>model</strong>. There<strong>for</strong>e it is important to carry out the rigorous<br />

<strong>simulations</strong> properly to ensure valid results are obtained.<br />

2.1 Mask defocus effect<br />

As EUV lithography uses a reflective <strong>mask</strong> illuminated with an oblique chief ray angle, the condition of telecentricity is<br />

no longer satisfied on the <strong>mask</strong> side as compared to DUV lithography. Consequently the effects of <strong>mask</strong> defocus are<br />

much more significant in EUV lithography. This aspect is particularly evident in lithography <strong>simulations</strong> using rigorous<br />

<strong>3D</strong> <strong>mask</strong> <strong>model</strong>s. In these <strong>simulations</strong> the transmitted (DUV) or reflected (EUV) <strong>mask</strong> fields are generally sampled at a<br />

pre-determined plane close to the top surface of the <strong>mask</strong> features. If these <strong>mask</strong> fields are directly used <strong>for</strong> subsequent<br />

image <strong>simulations</strong>, which implies that the sample plane is chosen as the object plane of the project lens, the images<br />

obtained at its conjugate image plane may not be optimum in terms of image contrast and pattern shift. As shown in<br />

Figure 1, the distance between the object plane and the sample plane is referred to as the <strong>mask</strong> defocus in this work.<br />

Multi -layer<br />

ens object plane<br />

sorber<br />

Mask defocus<br />

field sample plane<br />

Figure 1: Definition of <strong>mask</strong> defocus <strong>for</strong> this work<br />

From <strong>model</strong>ing point of view, the <strong>mask</strong> defocus effect may be ignored in DUV <strong>simulations</strong>, but it cannot be ignored in<br />

EUV <strong>simulations</strong>, especially <strong>for</strong> pattern shift. Note the effect of <strong>mask</strong> defocus is similar to wafer defocus but on a much<br />

smaller scale. It can be shown that the image change due to a <strong>mask</strong> defocus of m is approximately equivalent to a wafer<br />

defocus of w =M 2 m <strong>for</strong> low NA imaging, where M is the magnification of the projection lens. For a 4x reduction<br />

system, M 2 =1/16. For CD control this effect may be ignored or largely compensated by a small change in wafer defocus.<br />

But <strong>for</strong> pattern shift, it is a quite different situation between DUV and EUV.<br />

Many factors can contribute to the image shift of a pattern with respect to its position on the <strong>mask</strong>, including pattern<br />

symmetry, source symmetry, lens aberration, phase error induced by <strong>3D</strong> <strong>mask</strong> topography, <strong>mask</strong> defocus, wafer defocus,<br />

etc... We will only consider an aberration-free system in this work. For a symmetric pattern, it can be easily shown that<br />

the pattern shift caused by the defocus and/or <strong>3D</strong> <strong>mask</strong> topography can be cancelled out exactly by using a symmetric<br />

illumination pupil shape. This condition is generally satisfied in practical DUV applications. There<strong>for</strong>e the <strong>mask</strong> defocus<br />

effect rarely needs to be <strong>model</strong>ed in DUV <strong>simulations</strong>. However, due to the reflective <strong>mask</strong> and the oblique chief ray<br />

angle employed by EUV lithography, it is impossible to make a symmetric illumination pupil shape from the <strong>mask</strong><br />

viewpoint. As a result the pattern shift in EUV is not as trivial as in DUV. The contribution from the <strong>mask</strong> defocus is<br />

significant and generally global across all patterns. In addition, a <strong>mask</strong> pattern sees a slightly different illumination pupil<br />

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shape depending on its slit location. As a result, this global pattern shift on the field scale is shown as magnification error<br />

as a function of <strong>mask</strong> defocus.<br />

In practice, the global pattern shift is minimized during the scanner setup stage where the <strong>mask</strong> is driven to the optimum<br />

<strong>mask</strong> focal plane. It is important to <strong>model</strong> the same process in EUV <strong>simulations</strong> that use rigorous <strong>3D</strong> <strong>mask</strong> <strong>model</strong>s.<br />

Otherwise the resulting wafer image may show a large global pattern shift, which in reality is just a <strong>model</strong>ing artifact of<br />

not choosing the object plane properly. An example is shown in Figure 2, which compares the resist contours simulated<br />

by directly using the sample plane as the object plane to those simulated after moving the object plane to 180nm behind<br />

the sample plane. The <strong>mask</strong> <strong>simulations</strong> in this example were done using an ASML Brion in-house rigorous<br />

electromagnetic field (EMF) solver <strong>for</strong> Maxwell’s equations based on the FDTD method. A large global pattern shift of<br />

several nanometers is observed in simulation when the object plane is placed at the sample plane. But it can be corrected<br />

in simulation by moving the object plane to the optimum location, which mimics the scanner setup process.<br />

Note, <strong>for</strong> all the <strong>simulations</strong> presented in this work, an EUV system of numerical aperture NA=0.33, magnification<br />

M=0.25 and chief ray angle at object (CRAO) = 6 is used. The resist CDs and contours are computed from optical<br />

images using a constant threshold. No actual resist <strong>model</strong>s are used or required as the <strong>3D</strong> <strong>mask</strong> effects are optical effects.<br />

',ME<br />

It<br />

Object plane @ sample Iplane<br />

CD<br />

Object plane @ 180nm behind sample plane<br />

Slit location<br />

Le<br />

Illumination<br />

Bright-field<br />

image contour<br />

Dark-field<br />

image contour<br />

Figure 2: Comparison of the resist contours simulated by directly using the sample plane as the object plane (red<br />

contours) to those simulated after moving the object plane 180nm behind the sample plane (green contours)<br />

2.2 Incident angle effect<br />

In a lithography application the <strong>mask</strong> is generally illuminated by a partially coherent source. From <strong>model</strong>ing point of<br />

view, the source can be considered as a collection of planewaves, each is incoherent from others and illuminates the<br />

<strong>mask</strong> at a given incident angle. In low-NA DUV lithography <strong>simulations</strong>, the incident angle effect can be <strong>model</strong>ed using<br />

the so-called Hopkins approach, which assumes that the two transmitted fields produced by two plane waves of different<br />

angle of incidence differ by only a shift in spectral space. The diffraction order amplitude and relative phase remain the<br />

same. It is now well known that the Hopkins approach can introduce significant errors in high-NA DUV lithography<br />

<strong>simulations</strong> 8 . For the state-of-the-art DUV scanner of 1.35NA, the maximum angle of incidence on the <strong>mask</strong> is close to<br />

20 degrees. Rigorous <strong>mask</strong> <strong>simulations</strong> show that the relative phase in diffraction orders changes significantly over this<br />

range of angle of incidence. If not properly taken into account, it can produce wrong results in best focus shift<br />

predictions, which have been confirmed by both experiments and rigorous <strong>simulations</strong> 3 .<br />

The current most advanced EUV system under evaluation has NA of 0.33 and chief ray angle of 6 degrees. Figure 3<br />

shows the range of incident angle distribution on the EUV <strong>mask</strong> as compared to the DUV <strong>mask</strong>. Note the big circle in<br />

Figure 3 represents the maximum incident angle (~20 degrees) on the DUV <strong>mask</strong>. The center represents the normal<br />

incidence on the <strong>mask</strong>. The three smaller circles represent the range of the incident angle distribution on the EUV <strong>mask</strong><br />

<strong>for</strong> the slit center and two opposite edge locations, respectively. Since the incident angle distribution is much narrower<br />

on the EUV <strong>mask</strong>, it is reasonable to assume that the <strong>mask</strong> near field simulated at the chief ray angle may be<br />

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epresentative enough <strong>for</strong> the entire source. This turns out to be an acceptable assumption from CD and best focus<br />

prediction point of view. But it may not be adequate <strong>for</strong> pattern shift prediction depending on the accuracy requirement.<br />

DUV<br />

(Øuv<br />

-20°<br />

Figure 3: Comparison of the range of incident angle distribution on <strong>mask</strong> between EUV and DUV<br />

A straight<strong>for</strong>ward method to <strong>model</strong> the incident angle effect of a partially coherent illumination is to decompose the<br />

illumination pupil shape into smaller sections 9 . The angle of incidence is considered constant within each section and<br />

there<strong>for</strong>e only one rigorous <strong>3D</strong> <strong>mask</strong> simulation is required to compute its contribution to the wafer image using<br />

Hopkins approach. The total wafer image is the sum of the images produced by individual sections. The result is<br />

expected to converge as the number of sections increases.<br />

A simulation work was carried out to study the convergence as a function of the number of incident angles used <strong>for</strong><br />

rigorous EUV <strong>mask</strong> <strong>simulations</strong>. The illumination pupil shape and the incident angle locations are shown in Figure 4(a).<br />

The pupil shape is the same as that shown in Figure 2 and is used to illuminate the <strong>mask</strong> at the slit edge.<br />

r1 r1 r r:<br />

Figure 4(a): Pupil shape and incident angle locations used <strong>for</strong> rigorous <strong>3D</strong> <strong>mask</strong> <strong>simulations</strong><br />

We investigated both bright-field and dark-field <strong>mask</strong>s having horizontal (H) and vertical (V) lines or spaces of<br />

width=12nm and pitch=100nm on wafer scale. The simulation was done using HyperLith’s RCWA-based rigorous <strong>3D</strong><br />

<strong>mask</strong> <strong>model</strong>. We pre-scanned the <strong>mask</strong> defocus and selected a value to minimize the global patterns shift. This value was<br />

then fixed <strong>for</strong> all the <strong>simulations</strong>. Figure 4(b) shows the results of Bossung curves of XCD (CD of V line/space) and<br />

YCD (CD of H line/space). It is apparent that the number of angles has very small effect on CD and best focus shift. One<br />

angle of incidence at the chief ray may be considered adequate. It is also worth noting that the best focus shift is patterndependent<br />

between horizontal and vertical features, caused by <strong>3D</strong> <strong>mask</strong> topographies.<br />

Bright Field X & Y Bossung<br />

-100 -80 -60 -40 -20 0 20 40<br />

Wager Faune, nm<br />

60 80 100<br />

zcD_Mngles=l<br />

-XCD_Mngles=2<br />

-XCO_nAngles=4<br />

-XCD_nangles=12<br />

- XCD nAngles=l6<br />

-Y,11D_ A gl -<br />

-YCO_nAngles=2<br />

-0C11_44n0es=4<br />

- YCD Mngles=l2<br />

-YCD_Mngles=l6<br />

Dark Field X & Y Bossung<br />

-100 -80 -60 -40 -20 0 20 40 60<br />

Miler Foam, M<br />

80 100<br />

-XCO Mngles=l<br />

X00_44444=2<br />

XC0_nAngles=4<br />

XCD_nAndes=12<br />

-XCD_nAn41es=16<br />

-YCD_Mngles=l<br />

-1CD_Mngles=2<br />

-YCD_Mngles=4<br />

-VCD_Mngles=l2<br />

-YCD_Mngles=16<br />

Figure 4(b): Convergence of Bossung curve as a function of the number of incident angles used <strong>for</strong> rigorous <strong>3D</strong><br />

<strong>mask</strong> <strong>simulations</strong>. XCD = CD of V line/space. YCD = CD of H line/space.<br />

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Y Shift<br />

I<br />

Bright Field X & Y Shift thru Focus<br />

-Xshi t_nAnglesl<br />

X Shift<br />

-100 -80 -60 -40 -20 0 20 40 60 80 100<br />

wafeewas, nm<br />

-Xshift-nAngles =2<br />

Xshi t_nAngles4<br />

Xshift_nAnglesl2<br />

-Xshif[_nAngles16<br />

-Yshift _nAnelesl<br />

-Yshift_nAngles2<br />

-YshitLnAngles4<br />

-Yshift_nAngles12<br />

-YshilLnAngles16<br />

i<br />

C<br />

Dark Field X & Y Shift thru Focus<br />

Y Shift<br />

woji<br />

- 100 -80 -60 -40 -20 0 20 40 60 80 100<br />

Wafer Focus, mit<br />

-Xshift_nAndes=l<br />

-Xshift_nnndes=2<br />

-Xshift_nAngles4<br />

Xsliift_nAngles12<br />

-Xshift-nAngles=l6<br />

-Yshift-nAnglesl<br />

YshiR_nAngles=2<br />

-YShift _Mngles4<br />

-Yshi(t_Mnglesl2<br />

-YshilLMngles16<br />

Figure 4(c): Convergence of thru-focus pattern shift as a function of the number of incident angles used <strong>for</strong><br />

rigorous <strong>3D</strong> <strong>mask</strong> <strong>simulations</strong>. X Shift = pattern shift of V line/space. Y Shift = pattern shift of H line/space<br />

The convergence is however quite different <strong>for</strong> pattern shift. As shown in Figure 4(c), using only the chief ray angle can<br />

cause over 1nm error in pattern shift prediction and incorrect thru-focus trend. At least two incident angles, one <strong>for</strong> each<br />

pole, are required to reduce the error to below 0.5nm and to obtain the correct trend. More are needed to further reduce<br />

the error. But it is not going to be very practical <strong>for</strong> 2D pattern <strong>simulations</strong> as they are very time consuming. In this<br />

example, up to 12 incident angles may be required to obtain a near converged result.<br />

3. FAST <strong>3D</strong> MASK MODEL DEVELOPMENT<br />

In this section we describe the extension and enhancement of a fast approximate <strong>3D</strong> <strong>mask</strong> <strong>model</strong> <strong>for</strong> <strong>full</strong>-<strong>chip</strong> EUV<br />

applications. This <strong>model</strong> was developed previously <strong>for</strong> <strong>full</strong>-<strong>chip</strong> DUV applications and showed good accuracy in best<br />

focus shift predictions as compared to rigorous <strong>model</strong>s and experiments 3 . The details of its development are given in the<br />

previous work 10 and there<strong>for</strong>e not repeated here. In the following discussions, we first summarize the key elements of the<br />

previous <strong>model</strong> as they are the foundation of the present work. Then we describe the additional development made in<br />

this work to extend it <strong>for</strong> <strong>full</strong>-<strong>chip</strong> EUV applications.<br />

Figure 5: Illustration of the working principle of the fast <strong>3D</strong> <strong>mask</strong> <strong>model</strong><br />

As discussed in our previous work, the fast <strong>3D</strong> <strong>mask</strong> <strong>model</strong> developed <strong>for</strong> DUV lithography consists of the following<br />

key elements. First of all, the <strong>mask</strong> image of a given pattern is computed by convolving the layout properties such as<br />

polygon area and edges with the so-called M<strong>3D</strong> filters. This process is illustrated in Figure 5. For a coherent illumination<br />

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this <strong>mask</strong> image is directly related to the transmitted field of the <strong>mask</strong>. For a partially coherent illumination it does not<br />

have a direct association with a measureable physical property. It is more of an intermediate mathematical property that<br />

is to be convolved with the Transmission Cross Coefficient (TCC) of Hopkins theory to obtain the wafer image.<br />

There<strong>for</strong>e the <strong>model</strong> accuracy is determined by the <strong>mask</strong> image and in turn by the M<strong>3D</strong> filters. We construct these filters<br />

from a library of transmitted fields of representative <strong>mask</strong> features, pre-computed using a rigorous EMF solver <strong>for</strong><br />

Maxwell’s equations. The use of a rigorous EMF solver ensures that the relative phase between diffraction orders can be<br />

captured besides amplitude. Note this phase in<strong>for</strong>mation is completely missing in the thin <strong>mask</strong> <strong>model</strong> but plays an<br />

important role in determining the best focus of a given pattern. In addition, the relative phase greatly depends on the<br />

incident angle. In order to capture this dependency, an array of transmitted fields of various incident angles needs to be<br />

included in the rigorous library <strong>simulations</strong>. Then, <strong>for</strong> a given partially coherent illumination, we combine these rigorous<br />

library fields according to its pupil shape to compute the filters. The oblique incidence effect is thus embedded in these<br />

filters. One set of filters can be computed <strong>for</strong> the entire pupil or a sub-section of the pupil depending on the accuracy<br />

requirement. In a <strong>full</strong>-<strong>chip</strong> simulation these filters are re-used to compute the <strong>mask</strong> images <strong>for</strong> each patch of <strong>mask</strong><br />

patterns.<br />

It has been shown that the above <strong>model</strong> is capable of accurately predicting the best focus shift observed in rigorous<br />

<strong>simulations</strong> and experiments in DUV applications. In this work, it is further extended and enhanced <strong>for</strong> EUV<br />

applications. It is referred to as M<strong>3D</strong>+ <strong>model</strong> in this work as opposed to the previous M<strong>3D</strong> <strong>model</strong>. The basic working<br />

principle of this <strong>model</strong> stays the same as shown in Figure 5. The new developments are mainly in the area of M<strong>3D</strong>+<br />

filter generation that takes into account <strong>mask</strong> defocus effect and edge-to-edge interaction effect. These new<br />

developments are illustrated in Figure 6, followed by more detailed discussions on each of the components.<br />

Figure 6: Illustration of M<strong>3D</strong>+ filter generation <strong>for</strong> <strong>EUVL</strong> <strong>simulations</strong><br />

3.1 Library generation <strong>for</strong> EUV <strong>mask</strong><br />

EUV lithography uses a reflective <strong>mask</strong> as opposed to a transmissive <strong>mask</strong> in DUV lithography. There<strong>for</strong>e, instead of<br />

transmitted fields, the reflected fields of representative EUV <strong>mask</strong> features need to be rigorously simulated and stored in<br />

the library. The reflected fields at various incident angles, not just the chief ray angle, are also required in order to<br />

capture the incident angle effect of a partially coherent source in EUV lithography.<br />

3.2 Mask defocus<br />

As discussed in the previous section, the <strong>mask</strong> defocus has a significant effect on the results of EUV <strong>simulations</strong> with <strong>3D</strong><br />

<strong>mask</strong> <strong>model</strong>s. It is important to <strong>model</strong> the scanner setup process that moves the <strong>mask</strong> to the optimum <strong>mask</strong> focal plane.<br />

To enable this capability, the previous fast <strong>3D</strong> <strong>mask</strong> <strong>model</strong> is extended to include the <strong>mask</strong> defocus function. It is<br />

implemented by first propagating the library fields from the sample plane to the object plane as specified by the <strong>mask</strong><br />

defocus and then constructing the filters from the new library fields. Note that, since the <strong>mask</strong> defocus effect is included<br />

in the filters, there is no runtime impact in OPC and verification applications. The optimum <strong>mask</strong> defocus can be<br />

determined by mimicking the scanner setup process that minimizes the global pattern shift.<br />

Proc. of SPIE Vol. 8679 86790W-6<br />

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3.3 Edge-to-edge interaction<br />

From <strong>model</strong>ing point of view, the total EMF scattering effect of a <strong>mask</strong> may be separated into two parts – the primary<br />

scattering effect and the secondary scattering effect. The <strong>for</strong>mer refers to the EMF scattering effect of individual feature<br />

edges, including the interference effect of these individually scattered fields. The latter refers to the interaction effect that<br />

a scattered field being scattered again by nearby edges and so on. The secondary scattering effect is usually much<br />

smaller than the primary scattering effect. It may be ignored in many cases where the edge separation is large and/or the<br />

feature height is small so that the interaction is weak.<br />

As the device feature sizes continue to shrink, the <strong>model</strong>ing errors introduced by edge-to-edge interactions begin to show<br />

appreciable impact to the CD and overlay error budget. This effect is particularly apparent <strong>for</strong> EUV lithography because<br />

the absorber height is much larger than the wavelength and comparable to the spaces of dense features, making it more<br />

susceptible to interactions with the scattered fields from neighboring edges. The edge-to-edge interaction effect in EUV<br />

<strong>mask</strong> may be conceptually illustrated in Figure 7(a), where the largest arrow represents the incident field and the smaller<br />

solid arrows represent the primary scattered field from the left edge. Part of this scattered field hits the nearby right edge<br />

and is scattered again, resulting in a secondary scattered field.<br />

S<br />

Figure 7(a): Conceptual illustration of edge-toedge<br />

interaction in EUV <strong>mask</strong><br />

8 -<br />

7 -<br />

6 -<br />

5 -<br />

4 -<br />

3 -<br />

2 -<br />

1 -<br />

0<br />

1<br />

10<br />

Horizontal space CD error<br />

as a function of absorber space width<br />

- M<strong>3D</strong>+<br />

- M<strong>3D</strong><br />

15 20 25 30<br />

S @ wafer scale (nm)<br />

Illumination<br />

Figure 7(b): Model accuracy comparison between<br />

M<strong>3D</strong> (w/o edge-to-edge interaction effect taken<br />

into account) and M<strong>3D</strong>+ (w/ interaction effect<br />

taken into account)<br />

In this work we have extended the previous <strong>model</strong> by adding rigorous <strong>simulations</strong> of edge interaction fields as part of the<br />

library generation. These additional library fields enable us to extract the edge-to-edge interaction effect and build<br />

additional filters. By applying these filters we are able to include the edge-to-edge interaction effect in <strong>full</strong>-<strong>chip</strong> <strong>EUVL</strong><br />

<strong>simulations</strong>.<br />

A simulation example is shown in Figure 7(b) which compares the <strong>model</strong> accuracy as a function of absorber space<br />

between the M<strong>3D</strong> <strong>model</strong> (w/o the edge-to-edge interaction effect taken into account) and the M<strong>3D</strong>+ <strong>model</strong> (with the<br />

interaction effect taken into account). The CD error refers to the difference between the CD predicted by the<br />

M<strong>3D</strong>/M<strong>3D</strong>+ <strong>model</strong> and that by the rigorous FDTD <strong>model</strong>. As the space becomes smaller than 17nm (wafer scale), the<br />

M<strong>3D</strong> CD error starts to increase significantly while M<strong>3D</strong>+ maintains an excellent accuracy. The pitch is fixed at 100nm<br />

in this example. More accuracy evaluations on the M<strong>3D</strong>+ <strong>model</strong> are discussed in the next section.<br />

Note the above method <strong>for</strong> edge-to-edge interaction <strong>model</strong>ing is not limited to <strong>EUVL</strong>, it can be used <strong>for</strong> DUV<br />

<strong>simulations</strong> as well.<br />

4. MODEL ACCURACY VALIDATION<br />

In this section we evaluate the accuracy of the fast <strong>3D</strong> <strong>mask</strong> <strong>model</strong> against rigorous results <strong>for</strong> <strong>EUVL</strong> <strong>simulations</strong>. Two<br />

case studies were carried out, one on 1D patterns and the other on 2D patterns. The in-house FDTD EMF solver was<br />

used to generate the reference data <strong>for</strong> these studies as it is more memory efficient than RCWA <strong>for</strong> 2D pattern<br />

<strong>simulations</strong>. The benchmark between these two rigorous EMF solvers showed good agreement <strong>for</strong> the 1D test case<br />

presented in Section 2. The comparison is shown below in Figure 8.<br />

Proc. of SPIE Vol. 8679 86790W-7<br />

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Bright Field X & Y Bossung<br />

Dark Field X & Y Bossung<br />

XCD<br />

YCD<br />

XCDRCWA<br />

XCDFDID<br />

YCD RCWA<br />

-YCD FDID<br />

XCD<br />

/1111YCD<br />

XCDRCWA<br />

-XCDFDID<br />

-YCDRCWA<br />

-YCD FDID<br />

-100 -80 -60 -40 -20 0 20 40 60 80 100<br />

Wafer Pause, nm<br />

-100 -80 -60 -40 -20 0 20 40 60 80 100<br />

Wafer Focus, nm<br />

Bright Field X & Y Shift thru Focus<br />

Dark Field X & Y Shift thru Focus<br />

X Shift<br />

Y Shift<br />

-Xshlft RCWA<br />

-Wilk FIND<br />

-Yshift RCWA<br />

-YshBtFDTD<br />

s<br />

X Shift<br />

Y Shift<br />

-XShiftRCWA<br />

-XshiftFDTD<br />

-YshIft RCWA<br />

-Yshift FDlD<br />

-100 -80 40 -M -20 0 20 90 60 80 100<br />

Wafer roan, n<br />

-100 -80 40 -40 -20 0 20 90 60 80 100<br />

Wafer For. mr<br />

Figure 8: Comparison of simulation results between RCWA and FDTD<br />

In the following discussions we present the comparison between the fast <strong>3D</strong> <strong>mask</strong> <strong>model</strong> M<strong>3D</strong>+ and the rigorous <strong>3D</strong><br />

<strong>mask</strong> <strong>model</strong> FDTD. The comparison to thin <strong>mask</strong> <strong>model</strong> is also included as appropriate.<br />

4.1 1D pattern case study<br />

The 1D patterns used in this study consist of H/V lines (<strong>for</strong> bright-field <strong>mask</strong>) or spaces (<strong>for</strong> dark-field <strong>mask</strong>) of width<br />

from 10nm to 30nm, pitch from 28nm to 40nm with 2nm increment and from 40nm to 100nm with 10nm increment.<br />

Rigorous <strong>simulations</strong> were done first to generate the reference CD data <strong>for</strong> a range of focus-exposure matrix (FEM)<br />

conditions. The H and V line/space CD’s of the largest feature (i.e., 30nm lines or spaces with 100nm pitch) at the center<br />

slit location under the nominal FEM condition were used to calibrate the threshold of the M<strong>3D</strong>+ <strong>model</strong>. A thin <strong>mask</strong><br />

<strong>model</strong> was also calibrated, which included HV <strong>mask</strong> bias in addition to threshold. The calibrated <strong>model</strong> was then used to<br />

predict CDs and pattern shift of all features at both center and edge slit locations under the <strong>full</strong> range of FEM conditions.<br />

The results were compared with the rigorous reference data.<br />

Figure 9 shows the M<strong>3D</strong>+ and thin <strong>mask</strong> <strong>model</strong> RMS of predicted CD delta to rigorous FDTD <strong>model</strong>. The RMS was<br />

calculated across all features per slit location, FEM condition and <strong>mask</strong> type. The prediction power is significantly<br />

improved by the M<strong>3D</strong>+<strong>model</strong> over the thin <strong>mask</strong> <strong>model</strong>.<br />

The issue with the thin <strong>mask</strong> <strong>model</strong> is the lack of the prediction capability <strong>for</strong> pattern-dependent best focus shift and HV<br />

bias. An example is given in Figure 10, which compares the Bossung curves between the thin <strong>mask</strong> <strong>model</strong> and FDTD <strong>for</strong><br />

12nm and 30nm lines/spaces having 100nm pitch under the nominal dose condition. Clearly, the thin <strong>mask</strong> fails to<br />

capture the pattern-dependent best focus shift. In addition, the HV <strong>mask</strong> bias that works <strong>for</strong> large features fails to work<br />

<strong>for</strong> small features, particularly <strong>for</strong> the dark-field <strong>mask</strong>.<br />

The M<strong>3D</strong>+ is not shown in Figure 10 because it is on top of FDTD almost exactly in this example. More detailed<br />

Bossung comparisons between M<strong>3D</strong>+ and FDTD are given in Figures 11(a-d).<br />

The comparison of pattern shift between M<strong>3D</strong>+ and FDTD is shown in Figures 12(a-c). Thin <strong>mask</strong> <strong>model</strong> is not shown<br />

as it cannot capture this effect.<br />

Proc. of SPIE Vol. 8679 86790W-8<br />

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I<br />

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80-60-40-20 0 20 40 60<br />

Focus (nm)<br />

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Focus (nm)<br />

Focus (nm)<br />

- -<br />

-<br />

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80-60-40-20 0 20 40 60 80 80-60-40-20 0 20 40 60 80<br />

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Figure 9: M<strong>3D</strong>+ and thin <strong>mask</strong> <strong>model</strong> RMS of predicted CD delta to FDTD. The RMS was calculated across all<br />

features per slit location, FEM condition and <strong>mask</strong> type. The issue with the thin <strong>mask</strong> <strong>model</strong> is the lack of the<br />

prediction capability <strong>for</strong> pattern-dependent best focus shift and HV bias (see Figure 10).<br />

Comparison of Bossung between thin <strong>mask</strong> and FDTD<br />

Anchor<br />

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100<br />

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F Pitch (nm)<br />

Center<br />

Bright Field<br />

Edge<br />

Center<br />

Dark Field<br />

Edge<br />

F Slit Loc<br />

E- Mask Type<br />

Figure 10: Comparison of Bossung curves between thin <strong>mask</strong> <strong>model</strong> and FDTD under the nominal dose condition. The<br />

thin <strong>mask</strong> fails to capture the pattern-dependent best focus shift. In addition, the HV bias that works <strong>for</strong> large features<br />

in the thin <strong>mask</strong> <strong>model</strong> fails to work <strong>for</strong> small features, particularly <strong>for</strong> the dark-field <strong>mask</strong>.<br />

Proc. of SPIE Vol. 8679 86790W-9<br />

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Bright field thru -pitch Bossung of 12nm line at slit center<br />

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-80 0 80 -40 40 -80 0 80 -40 40 -80 0 80 -4040 -80 0 80 -40 40 -80 0 80 -40 40 -80 0 80 -40 40<br />

4- Focus (nm)<br />

30 32 34 36 38<br />

40 50 60 70<br />

80 90 100<br />

4- Pitch (nm)<br />

Figure 11(d): Dark field thru-pitch Bossung of 12nm space at slit edge under the nominal dose condition<br />

1.5<br />

Thru -pitch thru -focus Y pattern shift of<br />

12nm line /space at slit center<br />

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30 32 34 36 38 40 50 60 70 80 90 100<br />

F Focus (nm)<br />

F Pitch (nm)<br />

Figure 12(c): Dark field thru-pitch thru-focus pattern shift of 12nm space at slit edge under the nominal dose condition<br />

4.2 2D pattern case study<br />

2D patterns of an actual design are much more diverse compared to 1D patterns. To make this study more relevant, we<br />

adopted the 2D patterns previously investigated by a device manufacturer, which highlighted the need of <strong>3D</strong> <strong>mask</strong><br />

<strong>model</strong>ing in EUV applications 11 . These patterns are shown in Figure 13.<br />

EX1 (anchor)<br />

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Figure 13: 2D patterns used in simulation<br />

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The size of the feature at the simulation domain center is labeled. In this work these patterns were directly used in<br />

<strong>simulations</strong> without any OPC. Again, rigorous <strong>simulations</strong> were done first to generate reference data. The X- and Y-<br />

CD’s of the first pattern (EX1) at the slit center under the nominal FEM condition were used to calibrate the M<strong>3D</strong>+<br />

<strong>model</strong> and the thin <strong>mask</strong> <strong>model</strong>. Only threshold was calibrated <strong>for</strong> the M<strong>3D</strong>+ <strong>model</strong>. For the thin <strong>mask</strong> <strong>model</strong>, HV bias<br />

was also calibrated in addition to threshold. Then the calibrated <strong>model</strong> was used to predict the printed contours of all<br />

patterns and compared to rigorous results. The RMS of predicted CD delta to FDTD is shown in Figure 14.<br />

Proc. of SPIE Vol. 8679 86790W-12<br />

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Prediction F" IS (CD delta to FDTD)<br />

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Figure 14: M<strong>3D</strong>+ and thin <strong>mask</strong> <strong>model</strong> RMS of predicted CD delta to FDTD. The RMS was calculated across all<br />

features per slit location, FEM condition and <strong>mask</strong> type. One pattern was removed from the thin <strong>mask</strong> dark-field<br />

RMS calculation as it was not printed under the thin <strong>mask</strong> <strong>model</strong> (some thin <strong>mask</strong> <strong>model</strong> data points under offnominal<br />

conditions were also removed <strong>for</strong> the same reason).<br />

Note one pattern was removed from the thin <strong>mask</strong> dark-field RMS calculation as it was not printed under the thin <strong>mask</strong><br />

<strong>model</strong> (some thin <strong>mask</strong> <strong>model</strong> data points under off-nominal conditions were also removed <strong>for</strong> the same reason). But it<br />

was printed in the FDTD <strong>model</strong>. As shown in Figure 15 which compares the Bossung between thin <strong>mask</strong> and FDTD, the<br />

thin <strong>mask</strong> <strong>model</strong> CD of EX4B is reported as zero since the pattern fails to print. The dark-field <strong>mask</strong> generally has lower<br />

image quality, especially when without OPC, and there<strong>for</strong>e a small error in image can result in a large error in contour<br />

defined by threshold. For the same reason, the M<strong>3D</strong>+ <strong>model</strong> RMS is worse on the dark-field <strong>mask</strong> than the bright-field<br />

<strong>mask</strong>, although it is significantly improved over the thin <strong>mask</strong> <strong>model</strong>. More detailed comparisons between M<strong>3D</strong>+ and<br />

FDTD are given in Figure 16 on Bossung curves and in Figure 17 on pattern shift.<br />

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Figure 15: Dark field Bossung comparison between thin <strong>mask</strong> and FDTD under the nominal dose condition. Note<br />

the thin <strong>mask</strong> <strong>model</strong> CD of EX4B is reported as zero since the pattern fails to print. It was removed from the thin<br />

<strong>mask</strong> <strong>model</strong> RMS calculation.<br />

Proc. of SPIE Vol. 8679 86790W-13<br />

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Bright field Bossung comparison between M<strong>3D</strong>+ and FDTD<br />

Figure 16(a): Bright field Bossung comparison between M<strong>3D</strong>+ and FDTD under the nominal dose condition<br />

Dark field Bossung comparison between M<strong>3D</strong>+ and FDTD<br />

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Figure 16(b): Dark field Bossung comparison between M<strong>3D</strong>+ and FDTD under the nominal dose condition<br />

1.5<br />

Bright field thru -pitch pattern shift comparison between M<strong>3D</strong>+ and FDTD<br />

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Figure 17(a): Bright field pattern shift comparison between M<strong>3D</strong>+ and FDTD under the nominal dose condition<br />

Proc. of SPIE Vol. 8679 86790W-14<br />

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-1.5<br />

Dark field thru -pitch pattern shift comparison between M<strong>3D</strong>+ and FDTD<br />

_<br />

o<br />

.. _, .... ,..<br />

----'°- -- - '---<br />

O O ..,<br />

o<br />

o<br />

o<br />

:<br />

... .... ..<br />

%<br />

30 0 80 -40 40 -8,0 0 80 -40 40 -8,0 0 80 -40 40 -80 0 80 -40 40 -80 0 80 -40 40 -8,0 0 80 -40 40 -80 0 80 -40 40<br />

-XShift - FDTD<br />

o XShift - M<strong>3D</strong>+<br />

-YShift - FDTD<br />

o YShift-M<strong>3D</strong>+<br />

EX1<br />

EX1B<br />

EX2<br />

EX3<br />

EX4A<br />

EX4B<br />

EX4C<br />

EX1<br />

EX1B<br />

EX2<br />

EX3<br />

EX4A<br />

EX4B<br />

EX4C<br />

cntr<br />

edge<br />

Dark Field<br />

Figure 17(b): Dark field pattern shift comparison between M<strong>3D</strong>+ and FDTD under the nominal dose condition<br />

5. SUMMARY<br />

We have discussed the special considerations on <strong>mask</strong> defocus and incident angle effects in rigorous <strong>EUVL</strong> <strong>simulations</strong><br />

using <strong>3D</strong> <strong>mask</strong> <strong>model</strong>s. The optimum <strong>mask</strong> defocus needs to be determined first by mimicking the scanner setup process<br />

so that the global pattern shift or magnification error is minimized. Unlike in DUV <strong>simulations</strong>, the incident angle has<br />

only a small effect on CD and best focus prediction in EUV <strong>simulations</strong>. But it has a significant impact to pattern shift<br />

prediction.<br />

In this work we have extended and enhanced a fast <strong>3D</strong> <strong>mask</strong> <strong>model</strong> developed previously <strong>for</strong> <strong>full</strong>-<strong>chip</strong> DUV applications<br />

to EUV applications. The new development includes <strong>model</strong>ing of <strong>mask</strong> defocus and edge-to-edge interaction effects.<br />

Case studies were carried out to evaluate its accuracy against a rigorous <strong>3D</strong> <strong>mask</strong> <strong>model</strong> <strong>for</strong> 1D and 2D patterns in both<br />

bright-field and dark-field <strong>mask</strong>s. The fast <strong>3D</strong> <strong>mask</strong> <strong>model</strong> showed significant accuracy improvement over the thin <strong>mask</strong><br />

<strong>model</strong>. It accurately captured the Bossung shift/tilt as predicted by the rigorous <strong>model</strong>. It also captured the pattern shift<br />

within about 0.5nm error. It is worth pointing out that pattern shift <strong>simulations</strong> in general require more accurate <strong>model</strong>s.<br />

More improvement in this area may be needed depending on the overlay control requirement.<br />

ACKNOWLEDGMENT<br />

The authors would like to thank Ming Ding, Song Lan, Jun Chen and Mu Feng <strong>for</strong> their assistance in development and<br />

evaluation of the <strong>model</strong>.<br />

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