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Milster, Socha, BrookerSPIE- SC707
1
Basics of Optical Imaging in Microlithography: A "Hands-on" Approach
Tom D. Milster (University of Arizona)
Robert Socha (ASML)
Peter Brooker (SYNOPSYS)
Thanks to:• Del Hansen• Phat Lu•Warren Bletscher
Milster, Socha, BrookerSPIE- SC707
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What we want to do with this course
• Take a complicated optical system, like a lithographic projection camera used to make computer chips, and simplify it to a working model that demonstrates basic principles.
• Use a simple optical system for the student to work with “hands on” and observe the results.
• Demonstrate the relationship of the simple system to a real lithographic system through a commercial simulator.
• Have fun and demonstrate our unparalled acting abilities
From This To This
fc fcf1 f1 f2
f2 2fcam 2fcam
Condenser
Grating(Mask)
Lens 1
Stop
Lens 2
Image Plane (Aerial Image of Mask)
CCD Camera (AIMS)
SourceAperture
Milster, Socha, BrookerSPIE- SC707
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OUTLINE• Intro
– Basic Imaging – What we do in lithography– The goal of making a small image– What limits the size of the image?
• Basic Illumination and Imaging– Koehler Illumination– Definition of coherence factor “sigma”
• Binary Mask– Contrast versus pitch for sigma ~ 0– Contrast versus pitch for sigma > 0– 2-Beam and 3-Beam Imaging– Focus behavior
• Phase Mask– Contrast versus pitch– Focus behavior
• Off-Axis Illumination– Contrast versus pitch– Focus behavior
• Summary
Milster, Socha, BrookerSPIE- SC707
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Introduction• What is photo lithography ?
Etymology: Photolithography = Light Stone Writing
Photoresist Development
Negative Photoresist Positive Photoresist
Object: reticle or mask
Optics
Aerial ImagePhotoresist
Wafer + films Latent Image
• Optical image is recorded in the resist via changes in concentrations of species.
• Concentration level controls development
z
X
yResist Crosssections
Milster, Socha, BrookerSPIE- SC707
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Introduction• 1st approximation is that Aerial image propagates into photoresist normal to the wafer plane, creating a latent image• Reality is more complicated; you need to calculate E fields in photoresist at many propagation angles
0.25m 5-BAR Structures Focus=0.0m, NA=0.57 NA=0.6, 248nm
Image CrossSection
Resist CrossSection(not top down!)
Z
Z
Milster, Socha, BrookerSPIE- SC707
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Introduction• The goal of making a small image
– Transfer image into a photosensitive material, i.e., photoresist, for subsequent processing that results in a desired pattern to be used as a “stencil”
photoresist
Milster, Socha, BrookerSPIE- SC707
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Increase NA
Introduction• Imaging Resolution and Lord Rayleigh
– Q: When can you resolve the image of 2 distance stars?– A: When the 1st Intensity min of one lines up with peak of other
Decrease
Large NA
Web Top Optics, 1999
Resolution 0.61NA
Resolution 0.61
NA
Small NA
Large
From the math of the Airy function
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• Oh Master-Litho…• ..what limits the size of the photoresist pattern? • Grasshopper, there are three paths to improve resolution:
• Reduce Wavelength (Lambda)• Increase numerical aperture (NA)• Decrease k1 : “Process” knob
– Includes off-axis illumination, complex masks, high contrast photoresist, acid diffusion, etc…
• ….now go away Grasshopper I am busy.
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• What is it now Grasshopper…• Master, what affects the contrast of the image?• The answer is found in the values of
• NA• CD and Pitch• Partial Coherence or illumination (s)
– s=0: Coherent Limit– s=1: Incoherent Limit
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• You again grasshopper…• Master…• …look at the following data
Milster, Socha, BrookerSPIE- SC707
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100nm L/S
150nm L/S
Effect of Varying=193nm, NA=0.75
Dense Lines vs. (circular)
• Master, how come in one case increasing sigma is good (100nm L/S) and in the other case, increasing sigma is bad (200nm L/S)?
• It depends on the amount of diffraction orders that are being collected by the lens…now go away!
Milster, Socha, BrookerSPIE- SC707
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• Master, I am sure that your answers are correct but…• …yes Grasshopper…• But I find these facts confusing. What is sigma? How can in some
cases a larger sigma be good and in other cases a larger sigma be bad? And what the heck is k1?
• Master…I do not want only the answers…I want to understand…please help me understand master…
• Grasshopper… you are finally asking the right question• Go to the optical bench now…• It holds the answer to your questions!!
Milster, Socha, BrookerSPIE- SC707
fc fcf1 f1 f2
f2 2fcam 2fcam
LEDSource
Condenser
Grating(Mask)
Lens 1
Stop
Lens 2
Image Plane (Aerial Image of Mask)
CCD Camera (AIMS)
SourceAperture
First Light – Get An Image
Let’s do an experiment:– Set up the bench with:
• Pinhole Source• Aperture Stop of 6.35 mm (1/4 in) diameter.
− Put in the L (25.2µm) pitch mask and observe the aerial image.− The grating simulates a mask.− The aerial image simulates what is used to expose the resist.− In our system, the aerial image is reimaged onto a CCD camera, which is
like an Aerial Image Measurement System (AIMS).− Draw picture of the light pattern at the stop.
Milster, Socha, BrookerSPIE- SC707
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That is what your image looks like Draw the light pattern at the stop here.
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Basic Illumination and Imaging• Kohler Illumination
Condenser Imaging Lens
Mask PlaneSource
Aperture
Aerial Image
StopImage of source
• Field Stop of Imaging Lens is Aperture stop condenser and vice versa
• Lithographic systems use Koehler illumination where the illumination source aperture is imaged into the stop of the imaging lens.
Lens 1 Lens 2
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Basic Illumination and Imaging• Definition of Coherence Factor ‘Sigma’
CondenserImaging Lens
Mask Plane
Source
Stop Diameter
Source Image
Diameter
View of Entrance Pupil with blank mask
Pupil Edge (the “NA”)
Source Image
Diameter of Source Image in Stop
σDiameter of Stop
Milster, Socha, BrookerSPIE- SC707
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Simple Binary Mask• Model a Cr on quartz grating
mask as an infinitely thin grating
Position
E
SiO2
Cr
E-Field
P
0+1
+2
+3
-1
-2
-3Diffraction
Orders
Lens/Pupil
Grating Equation:
0th-1st +1st
Note: For 1:1 lines and spaces, P= 2 * LW
LW = Line Width
Pitch
)sin(
Milster, Socha, BrookerSPIE- SC707
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Effect of Varying Pitch
• Let’s do an experiment– Set up the bench with:
• Pinhole Source• Aperture Stop of 6.35 mm (1/4 in) diameter.
– Use the S(8.4µm), M(12.6µm) and L(25.2µm) pitches of the mask and observe the effects in the image plane and at the stop.
– Draw the light pattern at the stop on the next page.– What is the relationship between the light pattern at the stop and the
image?
– What is the smallest pitch for which we can obtain an image?
– This system is very similar to what would be observed if an on-axis laser beam was used to illuminate the mask. Therefore, we call this case coherent imaging.
– Notice that the lines in the image are either completely resolved, or they are not. There is no ‘partially resolved’ case.
Effect of Varying Pitch
Draw the light pattern at the stop for the S(8.4 µm) grating.
Draw the light pattern at the stop for the M(12.6 µm) grating.
Draw the light pattern at the stop for the L(25.2 µm) grating.
Milster, Socha, BrookerSPIE- SC707
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Milster, Socha, BrookerSPIE- SC707
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Binary Mask and Diffraction Orders
NAP
min min 2
LWNA
• Must have more than 1 order in pupil to have image modulation
Pupil (stop)
o
+1
+3
-3
-1
pupil
o
+1
-1
pupil
o
+1
-1
Coherent limit
No Image just constant Irradiance
For 1:1 grating
We see diffraction orders emanating from the mask that are necessary for imaging.
Pmin is the minimum pitch that is at the limit of resolution.
Max
NA=sin(Max)
Max
1Photoresist CD kNA
1Photoresist CD k
NA
k1=1/2
Strong Image Modulation
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Coffee Break
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• Time for the Late Shows new and exciting quiz game sensation.
• Do you want to play:– Know your “Current events”?
– Know your “Cuts of Beef’?
– Know your “Optics Bench Basics”?
• Know your Bench Basics! Excellent choice!!!
Milster, Socha, BrookerSPIE- SC707
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Bench basics:
• Where is the Source Aperture relative to the condenser lens?• Is it:• A: at minus infinity• B: it refuses to reveal its location• C: The source aperture is located at the front focus of the
condenser lens
• Answer is C: The source aperture (effective source for the system) is located at the focus of the condenser lens. Collimated light from the LED illuminates the grating. Light from every part of the source aperture illuminates each point on the grating.
Condenser
Grating(Mask)
Lens 1
Stop
Lens 2
Image Plane (Aerial Image of Mask)
CCD Camera (AIMS)
SourceAperture
fc fc f1 f1 f2f2 2fcam 2fcam
Milster, Socha, BrookerSPIE- SC707
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Bench basics
• Q: Where does the image of the Source Aperture appear?• Does it appear …• A: only in the Borg space time continuum• B: at the grating• C: in the plane of the “Stop”.
• Correct answer is C: The image of the Source Aperture appears in the plane of the stop.
fc fc f1 f1 f2f2 2fcam 2fcam
Condenser
Grating(Mask)
Lens 1
Stop
Lens 2
Image Plane (Aerial Image of Mask)
CCD Camera (AIMS)
SourceAperture
Milster, Socha, BrookerSPIE- SC707
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Bench basics
• Q: Collimated light from the Source Aperture illuminates the Grating. This is because….
• A: The grating is not worthy of the sources “focused” attention
• B: The source is the grating…question is irrelevant• C: Kohler Illumination of the grating averages out non
uniformities in the source.
• Answer is C
fc fc f1 f1 f2f2 2fcam 2fcam
Condenser
Grating(Mask)
Lens 1
Stop
Lens 2
Image Plane (Aerial Image of Mask)
CCD Camera (AIMS)
SourceAperture
Milster, Socha, BrookerSPIE- SC707
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• Comedy writer’s strike…
• No more multiple choice answers
• Let’s continue to cement the concepts associated with the bench
Milster, Socha, BrookerSPIE- SC707
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Bench Basics
• Q: Where is the grating located with respect to Lens1?• A: The grating is located at the focus of lens 1.
• Q: Where does the image of the grating appear?• A: The image of the grating appears at the “Image plane”
Condenser
Grating(Mask)
Lens 1
Stop
Lens 2
Image Plane (Aerial Image of Mask)
CCD Camera (AIMS)
SourceAperture
fc fc f1 f1 f2f2 2fcam 2fcam
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Bench Basics:
• Q: If the Image occurs at the image plane, why is the microscope needed?
• A: The image of the source at the image plane cannot be seen with the eye. The microscope is needed to magnify the image so it can be seen by your eye.
Condenser
Grating(Mask)
Lens 1
Stop
Lens 2
Image Plane (Aerial Image of Mask)
CCD Camera (AIMS)
SourceAperture
fc fc f1 f1 f2f2 2fcam 2fcam
Milster, Socha, BrookerSPIE- SC707
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Bench Basics: Grating off axis point
• Q: Look at the above picture. Estimate the vertical magnification?
• ~3.7
• How can the vertical magnification be decreased?• Decrease f2 but keep “Stop” at focus of Lens2.
f1 f1 f2 f2
Grating(Mask)
Lens 1
Stop
Lens 2
Image Plane (Aerial Image of Mask)
Milster, Socha, BrookerSPIE- SC707
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Connection back to real Scanner Optics
• Q: Where is the mask plane and image of the mask?• A: First plane on the left and last plane on right.
• Q: Can you find the stop in the lens column?• A: On the right side of center.
• Q: What is the magnification?• A: 4x demagnification.
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Effect of Varying Sigma• Let’s do an experiment
– Set up the bench with:• Pinhole Source• Aperture Stop of 6.35 mm diameter.• S(8.4µm) grating
– Use the PH, 3.18mm (1/8 in) and 6.35mm (1/4in) diameter sources and observe the effect at the stop and at the image plane. Estimate for each source.
– Draw the light pattern at the stop on the next page.– Is there a point where we can resolve the lines in the image?
– By changing , we are allowing more light through the stop that can interfere to form an image.
– Not all of the light that is passed through the stop can interfere, thus giving us background light that reduces our contrast. The amount of background light is a function of the pitch, therefore the contrast is a function of the pitch.
– This case is called partially coherent imaging, because of the dependence of the contrast on pitch.
Effect of Varying Sigma
Milster, Socha, BrookerSPIE- SC707
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Draw the light pattern at the stop for the PH light source.
Draw the light pattern at the stop for the 3.18mm diameter light
source.
Draw the light pattern at the stop for the 6.45mm diameter light
source.
Milster, Socha, BrookerSPIE- SC707
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Contrast Curves versus Pitch & Sigma
• Sigma=0.05 ---Coherent• Sigma=0.5 -----Partially Coherent• Sigma=1 ---Incoherent limit
Milster, Socha, BrookerSPIE- SC707
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Modulation Transfer Function (MTF)
• Optics types love this plot!!!!• Can you find the Coherent frequency cut off?
Milster, Socha, BrookerSPIE- SC707
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Binary Mask: Influence of Sigma
• Pupil diagrams with Partial Coherence :
No imaging Imaging!!
σ
NA’
• Each source point is projected by the diffraction orders from the mask – These will interfere with each other for a given source point– need more than 1 for interference and hence image modulation
We must have at least 2 conjugate sources points in the pupil to form an image.
Milster, Socha, BrookerSPIE- SC707
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Binary Mask: Sigma < 1
• No grating - just blank mask
0th order
0th order
-1st +1st
• Grating period at cut-off frequency
PNA
• Grating period resolution limit at given
min (1 )P
NA
0th order-1st +1st
limit 2 (1 )NA
Resolution limit with 0<<1 for a circular source
min
For 1:1 grating,
2 (1 )LW
NA
min 2LW
NA
Milster, Socha, BrookerSPIE- SC707
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Binary Mask: Sigma = 1
0th order• No grating - just
blank mask
-1st +1st
• Grating period at cut-off frequency
PNA
0th order-1st +1st
limitmin
4 2NAP
• Grating period corresponds to incoherent cut-off
min 2P
NA
Resolution limit with 1 for a circular source
min
For 1:1 grating,
4LW
NA
Milster, Socha, BrookerSPIE- SC707
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Binary Mask, =248nm, NA=0.63
Milster, Socha, BrookerSPIE- SC707
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=0.05 & = 0.7 for k1=0.5
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Different cases for on axis, k1=0.5
• Assume circular, on axis illumination• Assume dense L/S• k1=0.5
Center of n=1 diffraction orders are at edge of lens CD = LW = 0.5*Lambda/NA
• For 248nm illumination, NA=0.63– CD = 0.5*248nm/0.63 = 197nm 200nm L/S give k1=0.5
• For 193nm illumination, NA=0.93– CD = 0.5*193nm/0.93 = 104nm 104nm L/S give k1=0.5
• For 193nm illumination, NA = 1.2– CD = 0.5*193/1.2 = 80.4nm 80nm L/S gives k1 = 0.5
• Results above are only good for on axis illumination.• The usual off-axis case is different.
Milster, Socha, BrookerSPIE- SC707
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Binary Mask: Round and Annular Illumination
Larger and k1<0.5Small and k1>0.5
Conventional or Circular Source
Annular Source
• All power is inside pupil (for 0th and 1st orders)
• Coherent source points have 3-beam interaction
• Some power is inside pupil (center of 1st orders is outside)
• Coherent source points have 2-beam interaction
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Binary Mask: 3-Beam Imaging• Let’s do an experiment
– Set up the bench with:• L(25µm) Pitch grating• PH Source
– Observe the behavior (position and contrast) of the image as the observation plane is moved from the perfect focus. Write down your observations.
– What happens as the observation plane is moved beyond the point of zero contrast?
Binary Mask: 3-Beam Imaging– Do you see reversed-contrast lines?
– This type of focus behavior is indicative of three-beam imaging, where all of the power from the 0 and +/- 1st diffraction orders passes the stop.
– Every point in the image is derived from three conjugate source points in the pupil.
– Three-beam imaging has the characteristic that reversed-contrast planes can occur if the focus is too far or the resist is too thick.
Milster, Socha, BrookerSPIE- SC707
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Milster, Socha, BrookerSPIE- SC707
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Binary Mask, =248nm, NA=0.63, 300nm L/S
3-Beam Imaging
Milster, Socha, BrookerSPIE- SC707
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Missing Orders• Let’s do an experiment
– Set the bench with• L(25 µm) pitch• PH source
– Draw a sketch of the image on the next page.– Block the zero diffraction order at the stop.– Draw a sketch of the image on the next page.– Does the pitch of the image change?– This type of focus behavior is indicative of two-beam imaging.– Every point in the image is derived from two conjugate source
points in the pupil, which are widely separated and lead to a double-frequency image.
– Now change the system to block either the +1 or -1 order, but let the zero order pass the stop.
– Draw a sketch of the image on the next page.– Observe the image pitch and defocus behavior. Write down your
observations.
Missing Orders
L pitch and PH source Block zero order Block ± 1 order
Milster, Socha, BrookerSPIE- SC707
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Milster, Socha, BrookerSPIE- SC707
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Binary Mask, =248nm, NA=0.63, 250nm L/S
Milster, Socha, BrookerSPIE- SC707
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Phase MaskFor phase:
2( 1)d
n
E
E-Field
+1+3
+5
-1-3
-5Diffraction Orders
Lens/Pupil
Grating Equation:
-1st +1st
Cr
SiO2
Etched depth
d
Position
+1
-1
)(2
)sin(PitchCr
P
Milster, Socha, BrookerSPIE- SC707
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Pure Phase – Chromeless
E
E-Field
Diffraction Orders
Lens/Pupil
Position
+1
-1
SiO2
Etched depth
d
For phase: 2( 1)
dn
+1+3
+5
-1-3
-5
Grating Equation:
-1st +1st
Pitch
)sin(
P
Milster, Socha, BrookerSPIE- SC707
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Phase Mask• The phase mask produces no
zero order Pupil (stop)
+1
+3
-3
-1
pupil +1
-1
pupil
+1
-1
Coherent limit
No Image just constant Irradiance
Strong Image Modulation
No zero order is emitted from the phase mask.
pmin is the minimum Cr pitch that is at the limit of resolution.
min 4LW
NA
For alternating phase shift grating
NA=sin(Max)
Max
Max
NAP
2min
1Photoresist CD kNA
1Photoresist CD k
NA
k1=1/4
Milster, Socha, BrookerSPIE- SC707
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Phase Mask• Let’s do an experiment
– Set the bench with: .• 12.5µm Pitch Phase Mask• 14.25mm Diameter stop (No Magnet)• 3mm Diameter Source ( ~ 0.3)
– Observe the light pattern at the stop. How many diffraction orders do you see?
– Draw a sketch of image and the light pattern at the stop on the next page.– Note the relative brightness of the zero order and the +/-1st orders. If
needed, remove the grating to identify where the zero order occurs. – Observe the line pattern at the observation plane. (Block the zero order if
present)– How does the image pitch compare to using a simple grating mask?
Phase Mask– Change the observation plane location. How sensitive is the observation–
plane location to focus changes?
– The phase mask has no zero order, and it produces a double-frequency pitch in the aerial image compared to a binary mask.
– The minimum pitch in the image is half the minimum pitch of a simple grating mask.
– The phase-mask image is relatively insensitive to focus changes, due to the missing zero order.
Milster, Socha, BrookerSPIE- SC707
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Draw a sketch of image. Draw a sketch of light pattern at the stop.
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=248nm, NA=0.63, sigma = 0.3
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Off-Axis Illumination• Illumination source shapes that do not have axial intensity as usually known as off-axis sources
– Examples are annular, quadrupole, and dipole
• Off-axis illumination helps to enable k1<0.5 with binary masks– Reduction of on axis source reduces “DC” terms and enhances contrast
• A conventional on axis small source
Some Off-axis sources
Annular 45 Quadrupole 0 Quadrupole y- dipole x- dipole
Milster, Socha, BrookerSPIE- SC707
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Coherent Off-Axis Illumination and a Binary Mask• Orders shift relative to pupil
Image Modulation
pupil
0
+1
+3
-3
-1
0 Orderth
“Incoherent” limitpupil
0
-1
0 Orderth
pupil
0
-1
No Image just constant Irradiance
min 4LW
NA
For 1:1 grating
Max
Max
NA=sin(Max)
NAP
2min
1Photoresist CD kNA
1Photoresist CD k
NA
k1=1/4
Pmin is the minimum pitch that is at the limit of resolution.
Milster, Socha, BrookerSPIE- SC707
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Binary Mask with Annular Illumination
min
For 1:1 grating,
2 (1 )outer
LWNA
• No grating - just blank mask
-1st +1st
• Grating period at cut-off frequency
PNA
• Grating period resolution limit at given
min (1 )outer
PNA
-1st +1st
limit 2 (1 )outerNA
Resolution limit with 0<<1 for a circular source
inner
center
0th order
outer
0th order
0th order
Milster, Socha, BrookerSPIE- SC707
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Off-Axis Illumination with a Binary Mask• Let’s do an experiment
– Set up the bench with: system for minimum .
• S(8.2µm) pitch mask
• PH Source centered on axis
– Observe the pattern at the stop. Draw the light pattern at the stop on the next page.
– Do you see an image? Sketch the camera output on the next page.
– Move the source until at least two orders pass through the stop. Draw the pattern at the stop and the image on the next page.
Off-Axis Illumination with a Binary Mask
Draw a sketch with the centered source Draw a sketch with decentered source
Camera Output Camera Output
Milster, Socha, BrookerSPIE- SC707
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Milster, Socha, BrookerSPIE- SC707
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=248nm, NA=0.63, sigma = 0.3
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Different cases for off axis, k1=0.25
• Assume off axis illumination• Assume dense L/S• k1=0.25
Center of n=0 and n=1 diff. orders are at edge of lens CD = LW = 0.25*Lambda/NA
• For 248nm illumination, NA=0.63– CD = 0.5*248nm/0.63 = 98nm 100nm L/S give k1=0.25
• For 193nm illumination, NA=0.93– CD = 0.25*193nm/0.93 = 52nm 50nm L/S give k1=0.25
• For 193nm illumination, NA = 1.2– CD = 0.25*193/1.2 = 40.2nm 40nm L/S gives k1 = 0.25
• Current off-axis results.• Actually might want whole orders inside with sigma=0.3
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Summary• What have we learned?
– The basic optical components of a lithography system are the source, condenser and imaging lens.
– The size and shape of the source influence properties of the aerial image.
– The stop of the system determines the maximum angle of diffraction orders that can pass to the image.
– It takes at least two diffraction orders passing the stop to form a line-space image.
– By increasing , we can change from coherent-like illumination to partially-coherent illumination.
– Partially coherent illumination can allow higher pitch in the image at the expense of reduced contrast.
– 2-Beam and 3-Beam geometries have different focus characteristics.
– By using a phase-shift mask, the zero order is eliminated and the first diffraction orders move closer to the center.
– Off-axis illumination can produce a half-pitch image, but the contrast is lower than with a phase-shift mask.
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ReferencesIntroductory Articles
SPIE Proceedings for Microlithography
Journal of Microlithography, Microfabrication, and Microsystems (JM3) – SPIE Press
Industry MagazinesMicrolithography World
www.pennwell.com
BooksIntro to Fourier Optics and Statistical Optics
by J. GoodmanResolution Enhancement Techniques and Optical Imaging in Projection Microlithography
Alfred Wong, SPIE PressMicrolithography: Science and Technology
Ed: James Sheats and Bruce SmithPub: Marcel Dekker
Linear Systemsby J. Gaskill
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References
Intro Papers“Using location of diffraction orders to predict performance of future scanners”,
Peter Brooker Publication: Proc. SPIE Vol. 5256, p. 973-984, 23rd BACUS (2003) “Roles of NA, sigma, and lambda in low-k1 aerial image formation”,
Peter D. Brooker Publication: Proc. SPIE Vol. 4346, p. 1575-1586, (2001)
Advanced PapersU of A Dissertation by Doug Goodman (1979), Stationary Optical ProjectorsPapers by H.H. Hopkins for partial coherent imaging, Richards and Wolf for high NA
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Thank You for Taking This Course!
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Backup Slides
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Basic Illumination and Imaging
sin mNA n
NAh h
NA
• Pupil or “the aperture stop”: Physical Limiting aperture of system– Location and size defined by Chief Ray and Marginal Ray
• Chief Ray: Starts at edge of object (field) goes through center of pupil • Marginal Ray: Starts at axial object and goes through edge of pupil
Pupil
Aerial Image
Object
h’
h
n’ = image side refractive index
n = object side refractive index
Chief ray
Marginal ray
• NA: numerical aperture– defined by marginal ray
– maximum angle accepted by system
m
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Basic Illumination and Imaging
• Let’s do an experiment– Calculate NA at the image
plane for rs = _______ .
– Calculate the coherent
resolution limit in terms of pitch in the aerial image.
1
2
sin sin tan sm
rNA
f
rs
’m
2
1
________
525nm
n
f
sin mNA n
Imaging Lens
minpNA
Milster, Socha, BrookerSPIE- SC707
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Optimum DOF and Modulation for Annular (and dipole)
• Optimum when phase differences between 0th and 1st orders are minimum
center
/Pitch
1 1 1 1
2 4center Pitch NA LW NA
2 centerNAPitch
+1-1 0
Milster, Socha, BrookerSPIE- SC707
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Optimum DOF and Modulation for Quadrupole
• Optimum when phase differences between 0th and 1st orders are minimum
center
/Pitch
2 1 2 1
2 4center Pitch NA LW NA
22
centerNA
Pitch
+1-1 0
Milster, Socha, BrookerSPIE- SC707
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Periodic features benefit most from QUASAR illumination
Optimum illumination is specific to reticle features
conventional
annular
QUASARafter IMEC 1997
Resolution [/NA]2.01.51.00.50.0
0.0
0.5
1.0
1.5QUASAR hor. / vert.
QUASAR 45° lines
annular
conventional
DO
F [
µm
]
Dense Lines @ 60% contrast
Off-axis Illumination PrinciplesEffects of different illumination modes
Milster, Socha, BrookerSPIE- SC707
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More Facts: Aerial Image Cross Section
0.10
0.20
0.30
0.40
0.50
-100 -80 -60 -40 -20 0 20 40 60 80 100
Image Intensity
Horizontal Position (nm)
0.1
0.3
0.5
0.7
0.9
0.0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1.0
1.1
1.2
1.3
-100 0 100
Image Intensity
Horizontal Position (nm)
0.1
0.3
0.5
0.7
0.9
100nm L/S150nm L/S
Varying
=193nm, NA=0.75
Dense Lines vs. (circular)
• Increase sigma and contrast goes up (100nm L/S)• Increase sigma and contrast goes down (200 nm L/S)• Very confusing!!! What is going on??
Milster, Socha, BrookerSPIE- SC707
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Lithography Imaging Laws• What limits the size of the photoresist pattern ?
– Three paths to improve resolution:
• Wavelength ()
• Numerical Aperture (NA)
• k1 : “Process” knob
– Includes off-axis illumination, complex masks, high contrast photoresist, acid diffusion, etc…
• What limits the size of the optical (and/or aerial) image? (Assuming circular illumination source and binary reticle)
• NA• • Partial Coherence or illumination ()
– =0: Coherent Limit
– =1: Incoherent Limit
• Fine…but where do these come from??
1Photoresist CD kNA
1Photoresist CD k
NA
1Optical Resolution
2(1 ) NA
1Optical Resolution
2(1 ) NA
• Note: resolution is often written as Linewidth (LW) or critical dimension (CD) in the context with photoresist
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Basic Illumination and Imaging• Definition of Coherence Factor ‘Sigma’
CondenserImaging Lens
Mask Plane
Source
Stop Diameter
Source Image
Diameter
View of Entrance Pupil with blank mask
Pupil Edge (the “NA”)
Source Image
Diameter of Source Image in Stop
σDiameter of Stop
If pupil diameter = NA, then source size = NA • (pupil or NA units)