today’s outline - february 13, 2018phys.iit.edu/~segre/phys570/18s/lecture_11.pdf · today’s...
TRANSCRIPT
![Page 1: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/1.jpg)
Today’s Outline - February 13, 2018
• Ideal refractive surface
• Fresnel lenses and zone plates
• Research papers on refraction
• Kinematical diffraction
Homework Assignment #02:Problems on Blackboarddue Tuesday, February 13, 2018
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 1 / 23
![Page 2: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/2.jpg)
Today’s Outline - February 13, 2018
• Ideal refractive surface
• Fresnel lenses and zone plates
• Research papers on refraction
• Kinematical diffraction
Homework Assignment #02:Problems on Blackboarddue Tuesday, February 13, 2018
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 1 / 23
![Page 3: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/3.jpg)
Today’s Outline - February 13, 2018
• Ideal refractive surface
• Fresnel lenses and zone plates
• Research papers on refraction
• Kinematical diffraction
Homework Assignment #02:Problems on Blackboarddue Tuesday, February 13, 2018
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 1 / 23
![Page 4: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/4.jpg)
Today’s Outline - February 13, 2018
• Ideal refractive surface
• Fresnel lenses and zone plates
• Research papers on refraction
• Kinematical diffraction
Homework Assignment #02:Problems on Blackboarddue Tuesday, February 13, 2018
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 1 / 23
![Page 5: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/5.jpg)
Today’s Outline - February 13, 2018
• Ideal refractive surface
• Fresnel lenses and zone plates
• Research papers on refraction
• Kinematical diffraction
Homework Assignment #02:Problems on Blackboarddue Tuesday, February 13, 2018
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 1 / 23
![Page 6: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/6.jpg)
Today’s Outline - February 13, 2018
• Ideal refractive surface
• Fresnel lenses and zone plates
• Research papers on refraction
• Kinematical diffraction
Homework Assignment #02:Problems on Blackboarddue Tuesday, February 13, 2018
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 1 / 23
![Page 7: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/7.jpg)
Refractive optics
Just as with visible, light, it is possible to make refractive optics for x-rays
visible light:
n ∼ 1.2− 1.5f ∼ 0.1m
x-rays:
n ≈ 1− δ, δ ∼ 10−5
f ∼ 100m!
x-ray lenses are complementary to those for visible lightgetting manageable focal distances requires making compound lenses
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 2 / 23
![Page 8: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/8.jpg)
Refractive optics
Just as with visible, light, it is possible to make refractive optics for x-rays
visible light:
n ∼ 1.2− 1.5f ∼ 0.1m
x-rays:
n ≈ 1− δ, δ ∼ 10−5
f ∼ 100m!
x-ray lenses are complementary to those for visible lightgetting manageable focal distances requires making compound lenses
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 2 / 23
![Page 9: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/9.jpg)
Refractive optics
Just as with visible, light, it is possible to make refractive optics for x-rays
visible light:
n ∼ 1.2− 1.5f ∼ 0.1m
x-rays:
n ≈ 1− δ, δ ∼ 10−5
f ∼ 100m!
x-ray lenses are complementary to those for visible lightgetting manageable focal distances requires making compound lenses
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 2 / 23
![Page 10: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/10.jpg)
Refractive optics
Just as with visible, light, it is possible to make refractive optics for x-rays
visible light:
n ∼ 1.2− 1.5f ∼ 0.1m
x-rays:
n ≈ 1− δ, δ ∼ 10−5
f ∼ 100m!
x-ray lenses are complementary to those for visible light
getting manageable focal distances requires making compound lenses
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 2 / 23
![Page 11: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/11.jpg)
Refractive optics
Just as with visible, light, it is possible to make refractive optics for x-rays
visible light:
n ∼ 1.2− 1.5f ∼ 0.1m
x-rays:
n ≈ 1− δ, δ ∼ 10−5
f ∼ 100m!
x-ray lenses are complementary to those for visible lightgetting manageable focal distances requires making compound lenses
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 2 / 23
![Page 12: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/12.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal length
assuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 13: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/13.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f
→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 14: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/14.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 15: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/15.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1
→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 16: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/16.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f
→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 17: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/17.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 18: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/18.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2
→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 19: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/19.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f
→ i2 =f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 20: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/20.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 21: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/21.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2
→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 22: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/22.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f
→ i2 =f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 23: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/23.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 24: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/24.jpg)
Focal length of a compound lens
f1 f2 f3
1
i+
1
o=
1
f→ 1
i=
1
f− 1
o
1
i1=
1
f1− 1
o1→ 1
i1=
1
f→ i1 = f
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
1
f→ i2 =
f
2
1
i2=
1
f2− 1
o2→ 1
i2=
1
f+
2
f→ i2 =
f
3
Start with a 3-elementcompound lens, calculateeffective focal lengthassuming each lens hasthe same focal length, f
f1 = f , o1 =∞
for the second lens, theimage i1 is a virtualobject, o2 = −i1
similarly for the third lens,o3 = −i2
so for N lenses feff = f /N
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 3 / 23
![Page 25: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/25.jpg)
Rephasing distance
A spherical surface is not the ideal lens as it introduces aberrations. Derivethe ideal shape for perfect focusing of x-rays.
Λ
λο λ (1+δ)ο
consider two waves, one traveling in-side the solid and the other in vacuum,λ = λ0/(1− δ) ≈ λ0(1 + δ)
if the two waves start in phase, they will be in phaseonce again after a distance
Λ = (N + 1)λ0 = Nλ0(1 + δ)
Nλ0 + λ0 = Nλ0 + Nδλ0 −→ λ0 = Nδλ0 −→ N =1
δ
Λ = Nλ0 =λ0δ
=2π
λ0r0ρ≈ 10µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 4 / 23
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Rephasing distance
A spherical surface is not the ideal lens as it introduces aberrations. Derivethe ideal shape for perfect focusing of x-rays.
Λ
λο λ (1+δ)ο
consider two waves, one traveling in-side the solid and the other in vacuum,λ = λ0/(1− δ) ≈ λ0(1 + δ)
if the two waves start in phase, they will be in phaseonce again after a distance
Λ = (N + 1)λ0 = Nλ0(1 + δ)
Nλ0 + λ0 = Nλ0 + Nδλ0 −→ λ0 = Nδλ0 −→ N =1
δ
Λ = Nλ0 =λ0δ
=2π
λ0r0ρ≈ 10µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 4 / 23
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Rephasing distance
A spherical surface is not the ideal lens as it introduces aberrations. Derivethe ideal shape for perfect focusing of x-rays.
Λ
λο λ (1+δ)ο
consider two waves, one traveling in-side the solid and the other in vacuum,λ = λ0/(1− δ) ≈ λ0(1 + δ)
if the two waves start in phase, they will be in phaseonce again after a distance
Λ = (N + 1)λ0 = Nλ0(1 + δ)
Nλ0 + λ0 = Nλ0 + Nδλ0 −→ λ0 = Nδλ0 −→ N =1
δ
Λ = Nλ0 =λ0δ
=2π
λ0r0ρ≈ 10µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 4 / 23
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Rephasing distance
A spherical surface is not the ideal lens as it introduces aberrations. Derivethe ideal shape for perfect focusing of x-rays.
Λ
λο λ (1+δ)ο
consider two waves, one traveling in-side the solid and the other in vacuum,λ = λ0/(1− δ) ≈ λ0(1 + δ)
if the two waves start in phase, they will be in phaseonce again after a distance
Λ = (N + 1)λ0 = Nλ0(1 + δ)
Nλ0 + λ0 = Nλ0 + Nδλ0 −→ λ0 = Nδλ0 −→ N =1
δ
Λ = Nλ0 =λ0δ
=2π
λ0r0ρ≈ 10µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 4 / 23
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Rephasing distance
A spherical surface is not the ideal lens as it introduces aberrations. Derivethe ideal shape for perfect focusing of x-rays.
Λ
λο λ (1+δ)ο
consider two waves, one traveling in-side the solid and the other in vacuum,λ = λ0/(1− δ) ≈ λ0(1 + δ)
if the two waves start in phase, they will be in phaseonce again after a distance
Λ = (N + 1)λ0 = Nλ0(1 + δ)
Nλ0 + λ0 = Nλ0 + Nδλ0
−→ λ0 = Nδλ0 −→ N =1
δ
Λ = Nλ0 =λ0δ
=2π
λ0r0ρ≈ 10µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 4 / 23
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Rephasing distance
A spherical surface is not the ideal lens as it introduces aberrations. Derivethe ideal shape for perfect focusing of x-rays.
Λ
λο λ (1+δ)ο
consider two waves, one traveling in-side the solid and the other in vacuum,λ = λ0/(1− δ) ≈ λ0(1 + δ)
if the two waves start in phase, they will be in phaseonce again after a distance
Λ = (N + 1)λ0 = Nλ0(1 + δ)
Nλ0 + λ0 = Nλ0 + Nδλ0 −→ λ0 = Nδλ0
−→ N =1
δ
Λ = Nλ0 =λ0δ
=2π
λ0r0ρ≈ 10µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 4 / 23
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Rephasing distance
A spherical surface is not the ideal lens as it introduces aberrations. Derivethe ideal shape for perfect focusing of x-rays.
Λ
λο λ (1+δ)ο
consider two waves, one traveling in-side the solid and the other in vacuum,λ = λ0/(1− δ) ≈ λ0(1 + δ)
if the two waves start in phase, they will be in phaseonce again after a distance
Λ = (N + 1)λ0 = Nλ0(1 + δ)
Nλ0 + λ0 = Nλ0 + Nδλ0 −→ λ0 = Nδλ0 −→ N =1
δ
Λ = Nλ0 =λ0δ
=2π
λ0r0ρ≈ 10µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 4 / 23
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Rephasing distance
A spherical surface is not the ideal lens as it introduces aberrations. Derivethe ideal shape for perfect focusing of x-rays.
Λ
λο λ (1+δ)ο
consider two waves, one traveling in-side the solid and the other in vacuum,λ = λ0/(1− δ) ≈ λ0(1 + δ)
if the two waves start in phase, they will be in phaseonce again after a distance
Λ = (N + 1)λ0 = Nλ0(1 + δ)
Nλ0 + λ0 = Nλ0 + Nδλ0 −→ λ0 = Nδλ0 −→ N =1
δ
Λ = Nλ0 =λ0δ
=2π
λ0r0ρ≈ 10µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 4 / 23
![Page 33: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/33.jpg)
Rephasing distance
A spherical surface is not the ideal lens as it introduces aberrations. Derivethe ideal shape for perfect focusing of x-rays.
Λ
λο λ (1+δ)ο
consider two waves, one traveling in-side the solid and the other in vacuum,λ = λ0/(1− δ) ≈ λ0(1 + δ)
if the two waves start in phase, they will be in phaseonce again after a distance
Λ = (N + 1)λ0 = Nλ0(1 + δ)
Nλ0 + λ0 = Nλ0 + Nδλ0 −→ λ0 = Nδλ0 −→ N =1
δ
Λ = Nλ0 =λ0δ
=2π
λ0r0ρ
≈ 10µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 4 / 23
![Page 34: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/34.jpg)
Rephasing distance
A spherical surface is not the ideal lens as it introduces aberrations. Derivethe ideal shape for perfect focusing of x-rays.
Λ
λο λ (1+δ)ο
consider two waves, one traveling in-side the solid and the other in vacuum,λ = λ0/(1− δ) ≈ λ0(1 + δ)
if the two waves start in phase, they will be in phaseonce again after a distance
Λ = (N + 1)λ0 = Nλ0(1 + δ)
Nλ0 + λ0 = Nλ0 + Nδλ0 −→ λ0 = Nδλ0 −→ N =1
δ
Λ = Nλ0 =λ0δ
=2π
λ0r0ρ≈ 10µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 4 / 23
![Page 35: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/35.jpg)
Ideal interface profile
α
+x0
h(x)
λ ολ (1+δ)ο
∆x
A’A
B
B’
The wave exits thematerial into vacuumthrough a surface ofprofile h(x), and istwisted by an angle α.Follow the path of twopoints on the wave-front, A and A′ as theypropagate to B andB ′.
from the AA′B ′ trian-gle
and from the BCB ′ tri-angle
using Λ = λ0/δ
λ0 (1 + δ) = h′(x)∆x −→ ∆x ≈ λ0h′(x)
α(x) ≈ λ0δ
∆x= h′(x)δ = h′(x)
λ0Λ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 5 / 23
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Ideal interface profile
α
+x0
h(x)
λ ολ (1+δ)ο
∆x
A’A
B
B’
α
The wave exits thematerial into vacuumthrough a surface ofprofile h(x), and istwisted by an angle α.
Follow the path of twopoints on the wave-front, A and A′ as theypropagate to B andB ′.
from the AA′B ′ trian-gle
and from the BCB ′ tri-angle
using Λ = λ0/δ
λ0 (1 + δ) = h′(x)∆x −→ ∆x ≈ λ0h′(x)
α(x) ≈ λ0δ
∆x= h′(x)δ = h′(x)
λ0Λ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 5 / 23
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Ideal interface profile
α
+x0
h(x)
λ 0 λ (1+δ)0
∆x
A’A
B
B’
C
The wave exits thematerial into vacuumthrough a surface ofprofile h(x), and istwisted by an angle α.Follow the path of twopoints on the wave-front, A and A′ as theypropagate to B andB ′.
from the AA′B ′ trian-gle
and from the BCB ′ tri-angle
using Λ = λ0/δ
λ0 (1 + δ) = h′(x)∆x −→ ∆x ≈ λ0h′(x)
α(x) ≈ λ0δ
∆x= h′(x)δ = h′(x)
λ0Λ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 5 / 23
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Ideal interface profile
α
+x0
h(x)
λ 0 λ (1+δ)0
∆x
A’A
B
B’
C
The wave exits thematerial into vacuumthrough a surface ofprofile h(x), and istwisted by an angle α.Follow the path of twopoints on the wave-front, A and A′ as theypropagate to B andB ′.
from the AA′B ′ trian-gle
and from the BCB ′ tri-angle
using Λ = λ0/δ
λ0 (1 + δ) = h′(x)∆x −→ ∆x ≈ λ0h′(x)
α(x) ≈ λ0δ
∆x= h′(x)δ = h′(x)
λ0Λ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 5 / 23
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Ideal interface profile
α
+x0
h(x)
λ 0 λ (1+δ)0
∆x
A’A
B
B’
C
The wave exits thematerial into vacuumthrough a surface ofprofile h(x), and istwisted by an angle α.Follow the path of twopoints on the wave-front, A and A′ as theypropagate to B andB ′.
from the AA′B ′ trian-gle
and from the BCB ′ tri-angle
using Λ = λ0/δ
λ0 (1 + δ) = h′(x)∆x
−→ ∆x ≈ λ0h′(x)
α(x) ≈ λ0δ
∆x= h′(x)δ = h′(x)
λ0Λ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 5 / 23
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Ideal interface profile
α
+x0
h(x)
λ 0 λ (1+δ)0
∆x
A’A
B
B’
C
The wave exits thematerial into vacuumthrough a surface ofprofile h(x), and istwisted by an angle α.Follow the path of twopoints on the wave-front, A and A′ as theypropagate to B andB ′.
from the AA′B ′ trian-gle
and from the BCB ′ tri-angle
using Λ = λ0/δ
λ0 (1 + δ) = h′(x)∆x −→ ∆x ≈ λ0h′(x)
α(x) ≈ λ0δ
∆x= h′(x)δ = h′(x)
λ0Λ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 5 / 23
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Ideal interface profile
α
+x0
h(x)
λ 0 λ (1+δ)0
∆x
A’A
B
B’
C
The wave exits thematerial into vacuumthrough a surface ofprofile h(x), and istwisted by an angle α.Follow the path of twopoints on the wave-front, A and A′ as theypropagate to B andB ′.
from the AA′B ′ trian-gle
and from the BCB ′ tri-angle
using Λ = λ0/δ
λ0 (1 + δ) = h′(x)∆x −→ ∆x ≈ λ0h′(x)
α(x) ≈ λ0δ
∆x= h′(x)δ = h′(x)
λ0Λ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 5 / 23
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Ideal interface profile
α
+x0
h(x)
λ 0 λ (1+δ)0
∆x
A’A
B
B’
C
The wave exits thematerial into vacuumthrough a surface ofprofile h(x), and istwisted by an angle α.Follow the path of twopoints on the wave-front, A and A′ as theypropagate to B andB ′.
from the AA′B ′ trian-gle
and from the BCB ′ tri-angle
using Λ = λ0/δ
λ0 (1 + δ) = h′(x)∆x −→ ∆x ≈ λ0h′(x)
α(x) ≈ λ0δ
∆x
= h′(x)δ = h′(x)λ0Λ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 5 / 23
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Ideal interface profile
α
+x0
h(x)
λ 0 λ (1+δ)0
∆x
A’A
B
B’
C
The wave exits thematerial into vacuumthrough a surface ofprofile h(x), and istwisted by an angle α.Follow the path of twopoints on the wave-front, A and A′ as theypropagate to B andB ′.
from the AA′B ′ trian-gle
and from the BCB ′ tri-angle
using Λ = λ0/δ
λ0 (1 + δ) = h′(x)∆x −→ ∆x ≈ λ0h′(x)
α(x) ≈ λ0δ
∆x= h′(x)δ
= h′(x)λ0Λ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 5 / 23
![Page 44: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/44.jpg)
Ideal interface profile
α
+x0
h(x)
λ 0 λ (1+δ)0
∆x
A’A
B
B’
C
The wave exits thematerial into vacuumthrough a surface ofprofile h(x), and istwisted by an angle α.Follow the path of twopoints on the wave-front, A and A′ as theypropagate to B andB ′.
from the AA′B ′ trian-gle
and from the BCB ′ tri-angle
using Λ = λ0/δ
λ0 (1 + δ) = h′(x)∆x −→ ∆x ≈ λ0h′(x)
α(x) ≈ λ0δ
∆x= h′(x)δ
= h′(x)λ0Λ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 5 / 23
![Page 45: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/45.jpg)
Ideal interface profile
α
+x0
h(x)
λ 0 λ (1+δ)0
∆x
A’A
B
B’
C
The wave exits thematerial into vacuumthrough a surface ofprofile h(x), and istwisted by an angle α.Follow the path of twopoints on the wave-front, A and A′ as theypropagate to B andB ′.
from the AA′B ′ trian-gle
and from the BCB ′ tri-angle
using Λ = λ0/δ
λ0 (1 + δ) = h′(x)∆x −→ ∆x ≈ λ0h′(x)
α(x) ≈ λ0δ
∆x= h′(x)δ = h′(x)
λ0Λ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 5 / 23
![Page 46: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/46.jpg)
Ideal interface profile
If the desired focal length of this lens is f ,the wave must be redirected at an anglewhich depends on the distance from theoptical axis
α(x) =x
f
combining, we have
λ0h′(x)
Λ=
x
f−→ h′(x)
Λ=
x
f λ0
this can be directly integrated
h(x)
Λ=
x2
2f λ0=
[x√
2f λ0
]2
x0
α(x)f
a parabola is the ideal surfaceshape for focusing by refrac-tion
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 6 / 23
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Ideal interface profile
If the desired focal length of this lens is f ,the wave must be redirected at an anglewhich depends on the distance from theoptical axis
α(x) =x
f
combining, we have
λ0h′(x)
Λ=
x
f−→ h′(x)
Λ=
x
f λ0
this can be directly integrated
h(x)
Λ=
x2
2f λ0=
[x√
2f λ0
]2
x0
α(x)f
a parabola is the ideal surfaceshape for focusing by refrac-tion
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 6 / 23
![Page 48: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/48.jpg)
Ideal interface profile
If the desired focal length of this lens is f ,the wave must be redirected at an anglewhich depends on the distance from theoptical axis
α(x) =x
f
combining, we have
λ0h′(x)
Λ=
x
f
−→ h′(x)
Λ=
x
f λ0
this can be directly integrated
h(x)
Λ=
x2
2f λ0=
[x√
2f λ0
]2
x0
α(x)f
a parabola is the ideal surfaceshape for focusing by refrac-tion
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 6 / 23
![Page 49: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/49.jpg)
Ideal interface profile
If the desired focal length of this lens is f ,the wave must be redirected at an anglewhich depends on the distance from theoptical axis
α(x) =x
f
combining, we have
λ0h′(x)
Λ=
x
f−→ h′(x)
Λ=
x
f λ0
this can be directly integrated
h(x)
Λ=
x2
2f λ0=
[x√
2f λ0
]2
x0
α(x)f
a parabola is the ideal surfaceshape for focusing by refrac-tion
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 6 / 23
![Page 50: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/50.jpg)
Ideal interface profile
If the desired focal length of this lens is f ,the wave must be redirected at an anglewhich depends on the distance from theoptical axis
α(x) =x
f
combining, we have
λ0h′(x)
Λ=
x
f−→ h′(x)
Λ=
x
f λ0
this can be directly integrated
h(x)
Λ=
x2
2f λ0=
[x√
2f λ0
]2
x0
α(x)f
a parabola is the ideal surfaceshape for focusing by refrac-tion
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 6 / 23
![Page 51: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/51.jpg)
Ideal interface profile
If the desired focal length of this lens is f ,the wave must be redirected at an anglewhich depends on the distance from theoptical axis
α(x) =x
f
combining, we have
λ0h′(x)
Λ=
x
f−→ h′(x)
Λ=
x
f λ0
this can be directly integrated
h(x)
Λ=
x2
2f λ0
=
[x√
2f λ0
]2
x0
α(x)f
a parabola is the ideal surfaceshape for focusing by refrac-tion
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 6 / 23
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Ideal interface profile
If the desired focal length of this lens is f ,the wave must be redirected at an anglewhich depends on the distance from theoptical axis
α(x) =x
f
combining, we have
λ0h′(x)
Λ=
x
f−→ h′(x)
Λ=
x
f λ0
this can be directly integrated
h(x)
Λ=
x2
2f λ0=
[x√
2f λ0
]2x0
α(x)f
a parabola is the ideal surfaceshape for focusing by refrac-tion
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 6 / 23
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Ideal interface profile
If the desired focal length of this lens is f ,the wave must be redirected at an anglewhich depends on the distance from theoptical axis
α(x) =x
f
combining, we have
λ0h′(x)
Λ=
x
f−→ h′(x)
Λ=
x
f λ0
this can be directly integrated
h(x)
Λ=
x2
2f λ0=
[x√
2f λ0
]2x0
α(x)f
a parabola is the ideal surfaceshape for focusing by refrac-tion
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 6 / 23
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Focal length of circular lens
From the previous expression for the ideal parabolic surface, the focallength can be written in terms of the surface profile.
f =x2Λ
2λ0h(x)=
1
2δ
x2
h(x)or alternatively f =
1
δ
x
h′(x)
If the surface is a circle instead of a parabola
h(x) =√R2 − x2 and for x � R h(x) ≈ R
(1− 1
2
x2
R2
)
x2 = R2 − h2(x) ≈ R2 so we have f ≈ R
2δ
for N circular lenses
fn ≈R
2Nδ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 7 / 23
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Focal length of circular lens
From the previous expression for the ideal parabolic surface, the focallength can be written in terms of the surface profile.
f =x2Λ
2λ0h(x)
=1
2δ
x2
h(x)or alternatively f =
1
δ
x
h′(x)
If the surface is a circle instead of a parabola
h(x) =√R2 − x2 and for x � R h(x) ≈ R
(1− 1
2
x2
R2
)
x2 = R2 − h2(x) ≈ R2 so we have f ≈ R
2δ
for N circular lenses
fn ≈R
2Nδ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 7 / 23
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Focal length of circular lens
From the previous expression for the ideal parabolic surface, the focallength can be written in terms of the surface profile.
f =x2Λ
2λ0h(x)=
1
2δ
x2
h(x)
or alternatively f =1
δ
x
h′(x)
If the surface is a circle instead of a parabola
h(x) =√R2 − x2 and for x � R h(x) ≈ R
(1− 1
2
x2
R2
)
x2 = R2 − h2(x) ≈ R2 so we have f ≈ R
2δ
for N circular lenses
fn ≈R
2Nδ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 7 / 23
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Focal length of circular lens
From the previous expression for the ideal parabolic surface, the focallength can be written in terms of the surface profile.
f =x2Λ
2λ0h(x)=
1
2δ
x2
h(x)or alternatively f =
1
δ
x
h′(x)
If the surface is a circle instead of a parabola
h(x) =√R2 − x2 and for x � R h(x) ≈ R
(1− 1
2
x2
R2
)
x2 = R2 − h2(x) ≈ R2 so we have f ≈ R
2δ
for N circular lenses
fn ≈R
2Nδ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 7 / 23
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Focal length of circular lens
From the previous expression for the ideal parabolic surface, the focallength can be written in terms of the surface profile.
f =x2Λ
2λ0h(x)=
1
2δ
x2
h(x)or alternatively f =
1
δ
x
h′(x)
If the surface is a circle instead of a parabola
h(x) =√R2 − x2 and for x � R h(x) ≈ R
(1− 1
2
x2
R2
)
x2 = R2 − h2(x) ≈ R2 so we have f ≈ R
2δ
for N circular lenses
fn ≈R
2Nδ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 7 / 23
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Focal length of circular lens
From the previous expression for the ideal parabolic surface, the focallength can be written in terms of the surface profile.
f =x2Λ
2λ0h(x)=
1
2δ
x2
h(x)or alternatively f =
1
δ
x
h′(x)
If the surface is a circle instead of a parabola
h(x) =√R2 − x2
and for x � R h(x) ≈ R
(1− 1
2
x2
R2
)
x2 = R2 − h2(x) ≈ R2 so we have f ≈ R
2δ
for N circular lenses
fn ≈R
2Nδ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 7 / 23
![Page 60: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/60.jpg)
Focal length of circular lens
From the previous expression for the ideal parabolic surface, the focallength can be written in terms of the surface profile.
f =x2Λ
2λ0h(x)=
1
2δ
x2
h(x)or alternatively f =
1
δ
x
h′(x)
If the surface is a circle instead of a parabola
h(x) =√R2 − x2 and for x � R h(x) ≈ R
(1− 1
2
x2
R2
)
x2 = R2 − h2(x) ≈ R2 so we have f ≈ R
2δ
for N circular lenses
fn ≈R
2Nδ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 7 / 23
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Focal length of circular lens
From the previous expression for the ideal parabolic surface, the focallength can be written in terms of the surface profile.
f =x2Λ
2λ0h(x)=
1
2δ
x2
h(x)or alternatively f =
1
δ
x
h′(x)
If the surface is a circle instead of a parabola
h(x) =√R2 − x2 and for x � R h(x) ≈ R
(1− 1
2
x2
R2
)
x2 = R2 − h2(x) ≈ R2
so we have f ≈ R
2δ
for N circular lenses
fn ≈R
2Nδ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 7 / 23
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Focal length of circular lens
From the previous expression for the ideal parabolic surface, the focallength can be written in terms of the surface profile.
f =x2Λ
2λ0h(x)=
1
2δ
x2
h(x)or alternatively f =
1
δ
x
h′(x)
If the surface is a circle instead of a parabola
h(x) =√R2 − x2 and for x � R h(x) ≈ R
(1− 1
2
x2
R2
)
x2 = R2 − h2(x) ≈ R2 so we have f ≈ R
2δ
for N circular lenses
fn ≈R
2Nδ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 7 / 23
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Focal length of circular lens
From the previous expression for the ideal parabolic surface, the focallength can be written in terms of the surface profile.
f =x2Λ
2λ0h(x)=
1
2δ
x2
h(x)or alternatively f =
1
δ
x
h′(x)
If the surface is a circle instead of a parabola
h(x) =√R2 − x2 and for x � R h(x) ≈ R
(1− 1
2
x2
R2
)
x2 = R2 − h2(x) ≈ R2 so we have f ≈ R
2δ
for N circular lenses
fn ≈R
2Nδ
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 7 / 23
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Focussing by a beryllium lens
2R
d
unit lensf
For 50 holes of radius R = 1mm in beryllium (Be) at E = 10keV, we cancalculate the focal length, knowing δ = 3.41× 10−6
fN =R
2Nδ=
1× 10−3m
2(50)(3.41× 10−6)= 2.93m
depending on the wall thickness of the lenslets, the transmission can be upto 74%
H.R. Beguiristain et al., “X-ray focusing with compound lenses made from beryllium,” Optics Lett., 27, 778 (2007).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 8 / 23
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Focussing by a beryllium lens
2R
d
unit lensf
For 50 holes of radius R = 1mm in beryllium (Be) at E = 10keV, we cancalculate the focal length, knowing δ = 3.41× 10−6
fN =R
2Nδ
=1× 10−3m
2(50)(3.41× 10−6)= 2.93m
depending on the wall thickness of the lenslets, the transmission can be upto 74%
H.R. Beguiristain et al., “X-ray focusing with compound lenses made from beryllium,” Optics Lett., 27, 778 (2007).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 8 / 23
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Focussing by a beryllium lens
2R
d
unit lensf
For 50 holes of radius R = 1mm in beryllium (Be) at E = 10keV, we cancalculate the focal length, knowing δ = 3.41× 10−6
fN =R
2Nδ=
1× 10−3m
2(50)(3.41× 10−6)
= 2.93m
depending on the wall thickness of the lenslets, the transmission can be upto 74%
H.R. Beguiristain et al., “X-ray focusing with compound lenses made from beryllium,” Optics Lett., 27, 778 (2007).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 8 / 23
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Focussing by a beryllium lens
2R
d
unit lensf
For 50 holes of radius R = 1mm in beryllium (Be) at E = 10keV, we cancalculate the focal length, knowing δ = 3.41× 10−6
fN =R
2Nδ=
1× 10−3m
2(50)(3.41× 10−6)= 2.93m
depending on the wall thickness of the lenslets, the transmission can be upto 74%
H.R. Beguiristain et al., “X-ray focusing with compound lenses made from beryllium,” Optics Lett., 27, 778 (2007).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 8 / 23
![Page 68: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/68.jpg)
Focussing by a beryllium lens
2R
d
unit lensf
For 50 holes of radius R = 1mm in beryllium (Be) at E = 10keV, we cancalculate the focal length, knowing δ = 3.41× 10−6
fN =R
2Nδ=
1× 10−3m
2(50)(3.41× 10−6)= 2.93m
depending on the wall thickness of the lenslets, the transmission can be upto 74%
H.R. Beguiristain et al., “X-ray focusing with compound lenses made from beryllium,” Optics Lett., 27, 778 (2007).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 8 / 23
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Alligator-type lenses
Perhaps one of the most original x-ray lenses has been made by using oldvinyl records in an “alligator” configuration.
Bjorn Cederstrom et al., “Focusing hard X-rays with old LPs”, Nature 404, 951 (2000).
This design has also beenused to make lenses out oflithium metal.
E.M. Dufresne et al., “Lithium metal for x-ray refractive optics”, Appl. Phys. Lett. 79, 4085 (2001).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 9 / 23
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Alligator-type lenses
Perhaps one of the most original x-ray lenses has been made by using oldvinyl records in an “alligator” configuration.
Bjorn Cederstrom et al., “Focusing hard X-rays with old LPs”, Nature 404, 951 (2000).
This design has also beenused to make lenses out oflithium metal.
E.M. Dufresne et al., “Lithium metal for x-ray refractive optics”, Appl. Phys. Lett. 79, 4085 (2001).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 9 / 23
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Extruded Al lens
The compound refractive lenses (CRL) are useful for fixed focus but aredifficult to use if a variable focal distance and a long focal length isrequired.
Extruded aluminum lens withparabolic figure
Cut diagonally to exposevariable number of “lenses”to a horizontal beam
Horizontal translation allowschange in focal length but itis quantized, not continuous
A. Khounsary et al., “Fabrication, testing, and performance of a variable focus x-ray compound lens”, Proc. SPIE 4783, 49-54(2002).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 10 / 23
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Extruded Al lens
The compound refractive lenses (CRL) are useful for fixed focus but aredifficult to use if a variable focal distance and a long focal length isrequired.
Extruded aluminum lens withparabolic figure
Cut diagonally to exposevariable number of “lenses”to a horizontal beam
Horizontal translation allowschange in focal length but itis quantized, not continuous
A. Khounsary et al., “Fabrication, testing, and performance of a variable focus x-ray compound lens”, Proc. SPIE 4783, 49-54(2002).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 10 / 23
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Extruded Al lens
The compound refractive lenses (CRL) are useful for fixed focus but aredifficult to use if a variable focal distance and a long focal length isrequired.
Extruded aluminum lens withparabolic figure
Cut diagonally to exposevariable number of “lenses”to a horizontal beam
Horizontal translation allowschange in focal length but itis quantized, not continuous
A. Khounsary et al., “Fabrication, testing, and performance of a variable focus x-ray compound lens”, Proc. SPIE 4783, 49-54(2002).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 10 / 23
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Extruded Al lens
The compound refractive lenses (CRL) are useful for fixed focus but aredifficult to use if a variable focal distance and a long focal length isrequired.
Extruded aluminum lens withparabolic figure
Cut diagonally to exposevariable number of “lenses”to a horizontal beam
Horizontal translation allowschange in focal length but itis quantized, not continuous
A. Khounsary et al., “Fabrication, testing, and performance of a variable focus x-ray compound lens”, Proc. SPIE 4783, 49-54(2002).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 10 / 23
![Page 75: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/75.jpg)
Extruded Al lens
The compound refractive lenses (CRL) are useful for fixed focus but aredifficult to use if a variable focal distance and a long focal length isrequired.
Extruded aluminum lens withparabolic figure
Cut diagonally to exposevariable number of “lenses”to a horizontal beam
Horizontal translation allowschange in focal length but itis quantized, not continuous
A. Khounsary et al., “Fabrication, testing, and performance of a variable focus x-ray compound lens”, Proc. SPIE 4783, 49-54(2002).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 10 / 23
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Variable focal length CRL
A continuously variable focal length is very important for two specificreasons: tracking sample position, and keeping the focal length constantas energy is changed.
This can be achieved with a rotating lens system
Start with a 2 hole CRL. Rotate byan angle χ about vertical axis giv-ing an effective change in the num-ber of “lenses” by a factor 1/ cosχ.
at E = 5.5keV and χ = 0◦, heightis over 120µm
At χ = 30◦, it is under 50µm
Optimal focus is 20µm at χ = 40◦
B. Adams and C. Rose-Petruck, “X-ray focusing scheme with continuously variable lens,” J. Synchrotron Radiation 22, 16-22(2015).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 11 / 23
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Variable focal length CRL
A continuously variable focal length is very important for two specificreasons: tracking sample position, and keeping the focal length constantas energy is changed. This can be achieved with a rotating lens system
Start with a 2 hole CRL. Rotate byan angle χ about vertical axis giv-ing an effective change in the num-ber of “lenses” by a factor 1/ cosχ.
at E = 5.5keV and χ = 0◦, heightis over 120µm
At χ = 30◦, it is under 50µm
Optimal focus is 20µm at χ = 40◦
B. Adams and C. Rose-Petruck, “X-ray focusing scheme with continuously variable lens,” J. Synchrotron Radiation 22, 16-22(2015).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 11 / 23
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Variable focal length CRL
A continuously variable focal length is very important for two specificreasons: tracking sample position, and keeping the focal length constantas energy is changed. This can be achieved with a rotating lens system
Start with a 2 hole CRL.
Rotate byan angle χ about vertical axis giv-ing an effective change in the num-ber of “lenses” by a factor 1/ cosχ.
at E = 5.5keV and χ = 0◦, heightis over 120µm
At χ = 30◦, it is under 50µm
Optimal focus is 20µm at χ = 40◦
B. Adams and C. Rose-Petruck, “X-ray focusing scheme with continuously variable lens,” J. Synchrotron Radiation 22, 16-22(2015).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 11 / 23
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Variable focal length CRL
A continuously variable focal length is very important for two specificreasons: tracking sample position, and keeping the focal length constantas energy is changed. This can be achieved with a rotating lens system
Start with a 2 hole CRL. Rotate byan angle χ about vertical axis
giv-ing an effective change in the num-ber of “lenses” by a factor 1/ cosχ.
at E = 5.5keV and χ = 0◦, heightis over 120µm
At χ = 30◦, it is under 50µm
Optimal focus is 20µm at χ = 40◦
B. Adams and C. Rose-Petruck, “X-ray focusing scheme with continuously variable lens,” J. Synchrotron Radiation 22, 16-22(2015).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 11 / 23
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Variable focal length CRL
A continuously variable focal length is very important for two specificreasons: tracking sample position, and keeping the focal length constantas energy is changed. This can be achieved with a rotating lens system
Start with a 2 hole CRL. Rotate byan angle χ about vertical axis giv-ing an effective change in the num-ber of “lenses” by a factor 1/ cosχ.
at E = 5.5keV and χ = 0◦, heightis over 120µm
At χ = 30◦, it is under 50µm
Optimal focus is 20µm at χ = 40◦
B. Adams and C. Rose-Petruck, “X-ray focusing scheme with continuously variable lens,” J. Synchrotron Radiation 22, 16-22(2015).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 11 / 23
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Variable focal length CRL
A continuously variable focal length is very important for two specificreasons: tracking sample position, and keeping the focal length constantas energy is changed. This can be achieved with a rotating lens system
Start with a 2 hole CRL. Rotate byan angle χ about vertical axis giv-ing an effective change in the num-ber of “lenses” by a factor 1/ cosχ.
at E = 5.5keV and χ = 0◦, heightis over 120µm
At χ = 30◦, it is under 50µm
Optimal focus is 20µm at χ = 40◦
B. Adams and C. Rose-Petruck, “X-ray focusing scheme with continuously variable lens,” J. Synchrotron Radiation 22, 16-22(2015).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 11 / 23
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Variable focal length CRL
A continuously variable focal length is very important for two specificreasons: tracking sample position, and keeping the focal length constantas energy is changed. This can be achieved with a rotating lens system
Start with a 2 hole CRL. Rotate byan angle χ about vertical axis giv-ing an effective change in the num-ber of “lenses” by a factor 1/ cosχ.
at E = 5.5keV and χ = 0◦, heightis over 120µm
At χ = 30◦, it is under 50µm
Optimal focus is 20µm at χ = 40◦
B. Adams and C. Rose-Petruck, “X-ray focusing scheme with continuously variable lens,” J. Synchrotron Radiation 22, 16-22(2015).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 11 / 23
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Variable focal length CRL
A continuously variable focal length is very important for two specificreasons: tracking sample position, and keeping the focal length constantas energy is changed. This can be achieved with a rotating lens system
Start with a 2 hole CRL. Rotate byan angle χ about vertical axis giv-ing an effective change in the num-ber of “lenses” by a factor 1/ cosχ.
at E = 5.5keV and χ = 0◦, heightis over 120µm
At χ = 30◦, it is under 50µm
Optimal focus is 20µm at χ = 40◦
B. Adams and C. Rose-Petruck, “X-ray focusing scheme with continuously variable lens,” J. Synchrotron Radiation 22, 16-22(2015).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 11 / 23
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How to make a Fresnel lens
The ideal refracting lens has a parabolicshape (actually elliptical) but this is imprac-tical to make.
h(x) = Λ
(x√
2λo f
)2
when h(x) = 100Λ ∼ 1000µm
x = 10√
2λo f ∼ 100µm
aspect ratio too large for a stable structureand absorption would be too large!
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 12 / 23
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How to make a Fresnel lens
The ideal refracting lens has a parabolicshape (actually elliptical) but this is imprac-tical to make.
h(x) = Λ
(x√
2λo f
)2
when h(x) = 100Λ ∼ 1000µm
x = 10√
2λo f ∼ 100µm
aspect ratio too large for a stable structureand absorption would be too large!
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 12 / 23
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How to make a Fresnel lens
The ideal refracting lens has a parabolicshape (actually elliptical) but this is imprac-tical to make.
h(x) = Λ
(x√
2λo f
)2
when h(x) = 100Λ ∼ 1000µm
x = 10√
2λo f ∼ 100µm
aspect ratio too large for a stable structureand absorption would be too large!
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 12 / 23
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How to make a Fresnel lens
The ideal refracting lens has a parabolicshape (actually elliptical) but this is imprac-tical to make.
h(x) = Λ
(x√
2λo f
)2
when h(x) = 100Λ ∼ 1000µm
x = 10√
2λo f ∼ 100µm
aspect ratio too large for a stable structureand absorption would be too large!
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 12 / 23
![Page 88: Today’s Outline - February 13, 2018phys.iit.edu/~segre/phys570/18S/lecture_11.pdf · Today’s Outline - February 13, 2018 Ideal refractive surface Fresnel lenses and zone plates](https://reader033.vdocuments.us/reader033/viewer/2022042314/5f0231577e708231d4030887/html5/thumbnails/88.jpg)
How to make a Fresnel lens
The ideal refracting lens has a parabolicshape (actually elliptical) but this is imprac-tical to make.
h(x) = Λ
(x√
2λo f
)2
when h(x) = 100Λ ∼ 1000µm
x = 10√
2λo f ∼ 100µm
aspect ratio too large for a stable structureand absorption would be too large!
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 12 / 23
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How to make a Fresnel lens
Λ
2Λ
3Λ
4Λ
5Λ
6Λ
7Λ
Mark off the longitudinal zones (of thicknessΛ) where the waves inside and outside thematerial are in phase.
Each block of thickness Λ serves nopurpose for refraction but only attenuatesthe wave.
This material can be removed and theremaining material collapsed to producea Fresnel lens which has the same opticalproperties as the parabolic lens as long asf � NΛ where N is the number of zones.
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How to make a Fresnel lens
1
2
3
4
5
6
7
Mark off the longitudinal zones (of thicknessΛ) where the waves inside and outside thematerial are in phase.
Each block of thickness Λ serves nopurpose for refraction but only attenuatesthe wave.
This material can be removed and theremaining material collapsed to producea Fresnel lens which has the same opticalproperties as the parabolic lens as long asf � NΛ where N is the number of zones.
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 13 / 23
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How to make a Fresnel lens
1
2
3
4
5
6
7
Mark off the longitudinal zones (of thicknessΛ) where the waves inside and outside thematerial are in phase.
Each block of thickness Λ serves nopurpose for refraction but only attenuatesthe wave.
This material can be removed and theremaining material collapsed to producea Fresnel lens which has the same opticalproperties as the parabolic lens as long asf � NΛ where N is the number of zones.
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 13 / 23
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Fresnel lens dimensions
1
2
3
4
5
6
7 The outermost zones become very small andthus limit the overall aperture of the zoneplate. The dimensions of outermost zone, Ncan be calculated by first defining a scaledheight and lateral dimension
ν =h(x)
Λξ =
x√2λo f
Since ν = ξ2, the position of the Nth zoneis ξN =
√N and the scaled width of the Nth
(outermost) zone is
∆ξN = ξN − ξN−1 =√N −
√N − 1
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Fresnel lens dimensions
1
2
3
4
5
6
7 The outermost zones become very small andthus limit the overall aperture of the zoneplate. The dimensions of outermost zone, Ncan be calculated by first defining a scaledheight and lateral dimension
ν =h(x)
Λ
ξ =x√
2λo f
Since ν = ξ2, the position of the Nth zoneis ξN =
√N and the scaled width of the Nth
(outermost) zone is
∆ξN = ξN − ξN−1 =√N −
√N − 1
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 14 / 23
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Fresnel lens dimensions
1
2
3
4
5
6
7 The outermost zones become very small andthus limit the overall aperture of the zoneplate. The dimensions of outermost zone, Ncan be calculated by first defining a scaledheight and lateral dimension
ν =h(x)
Λξ =
x√2λo f
Since ν = ξ2, the position of the Nth zoneis ξN =
√N and the scaled width of the Nth
(outermost) zone is
∆ξN = ξN − ξN−1 =√N −
√N − 1
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 14 / 23
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Fresnel lens dimensions
1
2
3
4
5
6
7 The outermost zones become very small andthus limit the overall aperture of the zoneplate. The dimensions of outermost zone, Ncan be calculated by first defining a scaledheight and lateral dimension
ν =h(x)
Λξ =
x√2λo f
Since ν = ξ2, the position of the Nth zoneis ξN =
√N and the scaled width of the Nth
(outermost) zone is
∆ξN = ξN − ξN−1 =√N −
√N − 1
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 14 / 23
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Fresnel lens dimensions
1
2
3
4
5
6
7 The outermost zones become very small andthus limit the overall aperture of the zoneplate. The dimensions of outermost zone, Ncan be calculated by first defining a scaledheight and lateral dimension
ν =h(x)
Λξ =
x√2λo f
Since ν = ξ2, the position of the Nth zoneis ξN =
√N and the scaled width of the Nth
(outermost) zone is
∆ξN = ξN − ξN−1 =√N −
√N − 1
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 14 / 23
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Fresnel lens dimensions
1
2
3
4
5
6
7
∆ξN = ξN − ξN−1 =√N −
√N − 1
=√N
(1−
√1− 1
N
)
≈√N
(1−
[1− 1
2N
])∆ξN ≈
1
2√N
The diameter of the entire lens is thus
2ξN = 2√N =
1
∆ξN
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 15 / 23
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Fresnel lens dimensions
1
2
3
4
5
6
7
∆ξN = ξN − ξN−1 =√N −
√N − 1
=√N
(1−
√1− 1
N
)
≈√N
(1−
[1− 1
2N
])∆ξN ≈
1
2√N
The diameter of the entire lens is thus
2ξN = 2√N =
1
∆ξN
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 15 / 23
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Fresnel lens dimensions
1
2
3
4
5
6
7
∆ξN = ξN − ξN−1 =√N −
√N − 1
=√N
(1−
√1− 1
N
)
≈√N
(1−
[1− 1
2N
])
∆ξN ≈1
2√N
The diameter of the entire lens is thus
2ξN = 2√N =
1
∆ξN
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 15 / 23
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Fresnel lens dimensions
1
2
3
4
5
6
7
∆ξN = ξN − ξN−1 =√N −
√N − 1
=√N
(1−
√1− 1
N
)
≈√N
(1−
[1− 1
2N
])∆ξN ≈
1
2√N
The diameter of the entire lens is thus
2ξN = 2√N =
1
∆ξN
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 15 / 23
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Fresnel lens dimensions
1
2
3
4
5
6
7
∆ξN = ξN − ξN−1 =√N −
√N − 1
=√N
(1−
√1− 1
N
)
≈√N
(1−
[1− 1
2N
])∆ξN ≈
1
2√N
The diameter of the entire lens is thus
2ξN = 2√N =
1
∆ξN
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 15 / 23
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Fresnel lens example
In terms of the unscaled variables
∆xN = ∆ξN
√2λo f
=
√λo f
2N
dN = 2ξN =
√2λo f
∆ξN= 2√N√
2λo f =√
2Nλo f
If we take
λo = 1A = 1× 10−10m
f = 50cm = 0.5m
N = 100
∆xN = 5× 10−7m = 500nm dN = 2× 10−4m = 100µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 16 / 23
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Fresnel lens example
In terms of the unscaled variables
∆xN = ∆ξN
√2λo f =
√λo f
2N
dN = 2ξN =
√2λo f
∆ξN= 2√N√
2λo f =√
2Nλo f
If we take
λo = 1A = 1× 10−10m
f = 50cm = 0.5m
N = 100
∆xN = 5× 10−7m = 500nm dN = 2× 10−4m = 100µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 16 / 23
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Fresnel lens example
In terms of the unscaled variables
∆xN = ∆ξN
√2λo f =
√λo f
2N
dN = 2ξN
=
√2λo f
∆ξN= 2√N√
2λo f =√
2Nλo f
If we take
λo = 1A = 1× 10−10m
f = 50cm = 0.5m
N = 100
∆xN = 5× 10−7m = 500nm dN = 2× 10−4m = 100µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 16 / 23
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Fresnel lens example
In terms of the unscaled variables
∆xN = ∆ξN
√2λo f =
√λo f
2N
dN = 2ξN =
√2λo f
∆ξN
= 2√N√
2λo f =√
2Nλo f
If we take
λo = 1A = 1× 10−10m
f = 50cm = 0.5m
N = 100
∆xN = 5× 10−7m = 500nm dN = 2× 10−4m = 100µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 16 / 23
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Fresnel lens example
In terms of the unscaled variables
∆xN = ∆ξN
√2λo f =
√λo f
2N
dN = 2ξN =
√2λo f
∆ξN= 2√N√
2λo f =√
2Nλo f
If we take
λo = 1A = 1× 10−10m
f = 50cm = 0.5m
N = 100
∆xN = 5× 10−7m = 500nm dN = 2× 10−4m = 100µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 16 / 23
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Fresnel lens example
In terms of the unscaled variables
∆xN = ∆ξN
√2λo f =
√λo f
2N
dN = 2ξN =
√2λo f
∆ξN= 2√N√
2λo f =√
2Nλo f
If we take
λo = 1A = 1× 10−10m
f = 50cm = 0.5m
N = 100
∆xN = 5× 10−7m = 500nm dN = 2× 10−4m = 100µm
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 16 / 23
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Fresnel lens example
In terms of the unscaled variables
∆xN = ∆ξN
√2λo f =
√λo f
2N
dN = 2ξN =
√2λo f
∆ξN= 2√N√
2λo f =√
2Nλo f
If we take
λo = 1A = 1× 10−10m
f = 50cm = 0.5m
N = 100
∆xN = 5× 10−7m = 500nm
dN = 2× 10−4m = 100µm
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Fresnel lens example
In terms of the unscaled variables
∆xN = ∆ξN
√2λo f =
√λo f
2N
dN = 2ξN =
√2λo f
∆ξN= 2√N√
2λo f =√
2Nλo f
If we take
λo = 1A = 1× 10−10m
f = 50cm = 0.5m
N = 100
∆xN = 5× 10−7m = 500nm dN = 2× 10−4m = 100µm
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Making a Fresnel zone plate
Λ
Λ/2
The specific shape required for a zone plateis difficult to fabricate, consequently, itis convenient to approximate the nearlytriangular zones with a rectangular profile.
In practice, since the outermost zonesare very small, zone plates are generallyfabricated as alternating zones (rings for2D) of materials with a large Z-contrast,such as Au/Si or W/C.
This kind of zone plate is not as effi-cient as a true Fresnel lens would be in thex-ray regime. Nevertheless, efficiencies upto 35% have been achieved.
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Making a Fresnel zone plate
Λ
Λ/2
The specific shape required for a zone plateis difficult to fabricate, consequently, itis convenient to approximate the nearlytriangular zones with a rectangular profile.
In practice, since the outermost zonesare very small, zone plates are generallyfabricated as alternating zones (rings for2D) of materials with a large Z-contrast,such as Au/Si or W/C.
This kind of zone plate is not as effi-cient as a true Fresnel lens would be in thex-ray regime. Nevertheless, efficiencies upto 35% have been achieved.
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Making a Fresnel zone plate
Λ
Λ/2
The specific shape required for a zone plateis difficult to fabricate, consequently, itis convenient to approximate the nearlytriangular zones with a rectangular profile.
In practice, since the outermost zonesare very small, zone plates are generallyfabricated as alternating zones (rings for2D) of materials with a large Z-contrast,such as Au/Si or W/C.
This kind of zone plate is not as effi-cient as a true Fresnel lens would be in thex-ray regime. Nevertheless, efficiencies upto 35% have been achieved.
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 17 / 23
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Zone plate fabrication
Making high aspect ratio zone plates is challenging but a new process hasbeen developed to make plates with an aspect ratio as high as 25.
Start with Ultra nano crystallinediamond (UNCD) films on SiN.Coat with hydrogen silsesquioxane(HSQ). Pattern and develop theHSQ layer. Reactive ion etch theUNCD to the substrate. Plate withgold to make final zone plate.
The whole 150nm diameter zoneplate
Detail view of outer zones
SiN
UNCD
HSQ
M. Wojick et al., “X-ray zone plates with 25 aspect ratio using a 2-µm-thick ultrananocrystalline diamond mold,” Microsyst.Technol. 20, 2045-2050 (2014).
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Zone plate fabrication
Making high aspect ratio zone plates is challenging but a new process hasbeen developed to make plates with an aspect ratio as high as 25.
Start with Ultra nano crystallinediamond (UNCD) films on SiN.
Coat with hydrogen silsesquioxane(HSQ). Pattern and develop theHSQ layer. Reactive ion etch theUNCD to the substrate. Plate withgold to make final zone plate.
The whole 150nm diameter zoneplate
Detail view of outer zones
SiN
UNCD
HSQ
M. Wojick et al., “X-ray zone plates with 25 aspect ratio using a 2-µm-thick ultrananocrystalline diamond mold,” Microsyst.Technol. 20, 2045-2050 (2014).
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Zone plate fabrication
Making high aspect ratio zone plates is challenging but a new process hasbeen developed to make plates with an aspect ratio as high as 25.
Start with Ultra nano crystallinediamond (UNCD) films on SiN.Coat with hydrogen silsesquioxane(HSQ).
Pattern and develop theHSQ layer. Reactive ion etch theUNCD to the substrate. Plate withgold to make final zone plate.
The whole 150nm diameter zoneplate
Detail view of outer zones
SiN
UNCD
HSQ
M. Wojick et al., “X-ray zone plates with 25 aspect ratio using a 2-µm-thick ultrananocrystalline diamond mold,” Microsyst.Technol. 20, 2045-2050 (2014).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 18 / 23
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Zone plate fabrication
Making high aspect ratio zone plates is challenging but a new process hasbeen developed to make plates with an aspect ratio as high as 25.
Start with Ultra nano crystallinediamond (UNCD) films on SiN.Coat with hydrogen silsesquioxane(HSQ). Pattern and develop theHSQ layer.
Reactive ion etch theUNCD to the substrate. Plate withgold to make final zone plate.
The whole 150nm diameter zoneplate
Detail view of outer zones
SiN
UNCD
HSQ
M. Wojick et al., “X-ray zone plates with 25 aspect ratio using a 2-µm-thick ultrananocrystalline diamond mold,” Microsyst.Technol. 20, 2045-2050 (2014).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 18 / 23
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Zone plate fabrication
Making high aspect ratio zone plates is challenging but a new process hasbeen developed to make plates with an aspect ratio as high as 25.
Start with Ultra nano crystallinediamond (UNCD) films on SiN.Coat with hydrogen silsesquioxane(HSQ). Pattern and develop theHSQ layer. Reactive ion etch theUNCD to the substrate.
Plate withgold to make final zone plate.
The whole 150nm diameter zoneplate
Detail view of outer zones
SiN
UNCD
HSQ
M. Wojick et al., “X-ray zone plates with 25 aspect ratio using a 2-µm-thick ultrananocrystalline diamond mold,” Microsyst.Technol. 20, 2045-2050 (2014).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 18 / 23
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Zone plate fabrication
Making high aspect ratio zone plates is challenging but a new process hasbeen developed to make plates with an aspect ratio as high as 25.
Start with Ultra nano crystallinediamond (UNCD) films on SiN.Coat with hydrogen silsesquioxane(HSQ). Pattern and develop theHSQ layer. Reactive ion etch theUNCD to the substrate. Plate withgold to make final zone plate.
The whole 150nm diameter zoneplate
Detail view of outer zones
SiN
UNCD
HSQ
M. Wojick et al., “X-ray zone plates with 25 aspect ratio using a 2-µm-thick ultrananocrystalline diamond mold,” Microsyst.Technol. 20, 2045-2050 (2014).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 18 / 23
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Zone plate fabrication
Making high aspect ratio zone plates is challenging but a new process hasbeen developed to make plates with an aspect ratio as high as 25.
Start with Ultra nano crystallinediamond (UNCD) films on SiN.Coat with hydrogen silsesquioxane(HSQ). Pattern and develop theHSQ layer. Reactive ion etch theUNCD to the substrate. Plate withgold to make final zone plate.
The whole 150nm diameter zoneplate
Detail view of outer zones
SiN
UNCD
HSQ
M. Wojick et al., “X-ray zone plates with 25 aspect ratio using a 2-µm-thick ultrananocrystalline diamond mold,” Microsyst.Technol. 20, 2045-2050 (2014).
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 18 / 23
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Zone plate fabrication
Making high aspect ratio zone plates is challenging but a new process hasbeen developed to make plates with an aspect ratio as high as 25.
Start with Ultra nano crystallinediamond (UNCD) films on SiN.Coat with hydrogen silsesquioxane(HSQ). Pattern and develop theHSQ layer. Reactive ion etch theUNCD to the substrate. Plate withgold to make final zone plate.
The whole 150nm diameter zoneplate
Detail view of outer zones
SiN
UNCD
HSQ
M. Wojick et al., “X-ray zone plates with 25 aspect ratio using a 2-µm-thick ultrananocrystalline diamond mold,” Microsyst.Technol. 20, 2045-2050 (2014).
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Scattering from two electrons
Consider systems where there is only weak scattering, with no multiplescattering effects. We begin with the scattering of x-rays from twoelectrons.
r
2θ
k
k
2θ
Q
k
k
~Q = (~k − ~k ′)
|~Q| = 2k sin θ =4π
λsin θ
The scattering from the second electron willhave a phase shift of φ = ~Q ·~r .
A(~Q) = −r0(
1 + e i ~Q·~r)
I (~Q) = A(~Q)∗A(~Q)
= r20
(1 + e i ~Q·~r
)(1 + e−i ~Q·~r
)I (~Q) = r20
(1 + e i ~Q·~r + e−i ~Q·~r + 1
)= 2r20
(1 + cos(~Q ·~r)
)
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Scattering from two electrons
Consider systems where there is only weak scattering, with no multiplescattering effects. We begin with the scattering of x-rays from twoelectrons.
r
2θ
k
k
2θ
Q
k
k
~Q = (~k − ~k ′)
|~Q| = 2k sin θ =4π
λsin θ
The scattering from the second electron willhave a phase shift of φ = ~Q ·~r .
A(~Q) = −r0(
1 + e i ~Q·~r)
I (~Q) = A(~Q)∗A(~Q)
= r20
(1 + e i ~Q·~r
)(1 + e−i ~Q·~r
)I (~Q) = r20
(1 + e i ~Q·~r + e−i ~Q·~r + 1
)= 2r20
(1 + cos(~Q ·~r)
)
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Scattering from two electrons
Consider systems where there is only weak scattering, with no multiplescattering effects. We begin with the scattering of x-rays from twoelectrons.
r
2θ
k
k
2θ
Q
k
k
~Q = (~k − ~k ′)
|~Q| = 2k sin θ =4π
λsin θ
The scattering from the second electron willhave a phase shift of φ = ~Q ·~r .
A(~Q) = −r0(
1 + e i ~Q·~r)
I (~Q) = A(~Q)∗A(~Q)
= r20
(1 + e i ~Q·~r
)(1 + e−i ~Q·~r
)I (~Q) = r20
(1 + e i ~Q·~r + e−i ~Q·~r + 1
)= 2r20
(1 + cos(~Q ·~r)
)
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Scattering from two electrons
Consider systems where there is only weak scattering, with no multiplescattering effects. We begin with the scattering of x-rays from twoelectrons.
r
2θ
k
k
2θ
Q
k
k
~Q = (~k − ~k ′)
|~Q| = 2k sin θ =4π
λsin θ
The scattering from the second electron willhave a phase shift of φ = ~Q ·~r .
A(~Q) = −r0(
1 + e i ~Q·~r)
I (~Q) = A(~Q)∗A(~Q)
= r20
(1 + e i ~Q·~r
)(1 + e−i ~Q·~r
)I (~Q) = r20
(1 + e i ~Q·~r + e−i ~Q·~r + 1
)= 2r20
(1 + cos(~Q ·~r)
)
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Scattering from two electrons
Consider systems where there is only weak scattering, with no multiplescattering effects. We begin with the scattering of x-rays from twoelectrons.
r
2θ
k
k
2θ
Q
k
k
~Q = (~k − ~k ′)
|~Q| = 2k sin θ =4π
λsin θ
The scattering from the second electron willhave a phase shift of φ = ~Q ·~r .
A(~Q) = −r0(
1 + e i ~Q·~r)
I (~Q) = A(~Q)∗A(~Q)
= r20
(1 + e i ~Q·~r
)(1 + e−i ~Q·~r
)I (~Q) = r20
(1 + e i ~Q·~r + e−i ~Q·~r + 1
)= 2r20
(1 + cos(~Q ·~r)
)
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Scattering from two electrons
Consider systems where there is only weak scattering, with no multiplescattering effects. We begin with the scattering of x-rays from twoelectrons.
r
2θ
k
k
2θ
Q
k
k
~Q = (~k − ~k ′)
|~Q| = 2k sin θ =4π
λsin θ
The scattering from the second electron willhave a phase shift of φ = ~Q ·~r .
A(~Q) = −r0(
1 + e i ~Q·~r)
I (~Q) = A(~Q)∗A(~Q)
= r20
(1 + e i ~Q·~r
)(1 + e−i ~Q·~r
)I (~Q) = r20
(1 + e i ~Q·~r + e−i ~Q·~r + 1
)= 2r20
(1 + cos(~Q ·~r)
)
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Scattering from two electrons
Consider systems where there is only weak scattering, with no multiplescattering effects. We begin with the scattering of x-rays from twoelectrons.
r
2θ
k
k
2θ
Q
k
k
~Q = (~k − ~k ′)
|~Q| = 2k sin θ =4π
λsin θ
The scattering from the second electron willhave a phase shift of φ = ~Q ·~r .
A(~Q) = −r0(
1 + e i ~Q·~r)
I (~Q) = A(~Q)∗A(~Q)
= r20
(1 + e i ~Q·~r
)(1 + e−i ~Q·~r
)I (~Q) = r20
(1 + e i ~Q·~r + e−i ~Q·~r + 1
)= 2r20
(1 + cos(~Q ·~r)
)
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Scattering from two electrons
Consider systems where there is only weak scattering, with no multiplescattering effects. We begin with the scattering of x-rays from twoelectrons.
r
2θ
k
k
2θ
Q
k
k
~Q = (~k − ~k ′)
|~Q| = 2k sin θ =4π
λsin θ
The scattering from the second electron willhave a phase shift of φ = ~Q ·~r .
A(~Q) = −r0(
1 + e i ~Q·~r)
I (~Q) = A(~Q)∗A(~Q)
= r20
(1 + e i ~Q·~r
)(1 + e−i ~Q·~r
)I (~Q) = r20
(1 + e i ~Q·~r + e−i ~Q·~r + 1
)= 2r20
(1 + cos(~Q ·~r)
)
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Scattering from two electrons
Consider systems where there is only weak scattering, with no multiplescattering effects. We begin with the scattering of x-rays from twoelectrons.
r
2θ
k
k
2θ
Q
k
k
~Q = (~k − ~k ′)
|~Q| = 2k sin θ =4π
λsin θ
The scattering from the second electron willhave a phase shift of φ = ~Q ·~r .
A(~Q) = −r0(
1 + e i ~Q·~r)
I (~Q) = A(~Q)∗A(~Q)
= r20
(1 + e i ~Q·~r
)(1 + e−i ~Q·~r
)
I (~Q) = r20
(1 + e i ~Q·~r + e−i ~Q·~r + 1
)= 2r20
(1 + cos(~Q ·~r)
)
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Scattering from two electrons
Consider systems where there is only weak scattering, with no multiplescattering effects. We begin with the scattering of x-rays from twoelectrons.
r
2θ
k
k
2θ
Q
k
k
~Q = (~k − ~k ′)
|~Q| = 2k sin θ =4π
λsin θ
The scattering from the second electron willhave a phase shift of φ = ~Q ·~r .
A(~Q) = −r0(
1 + e i ~Q·~r)
I (~Q) = A(~Q)∗A(~Q)
= r20
(1 + e i ~Q·~r
)(1 + e−i ~Q·~r
)I (~Q) = r20
(1 + e i ~Q·~r + e−i ~Q·~r + 1
)
= 2r20
(1 + cos(~Q ·~r)
)
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Scattering from two electrons
Consider systems where there is only weak scattering, with no multiplescattering effects. We begin with the scattering of x-rays from twoelectrons.
r
2θ
k
k
2θ
Q
k
k
~Q = (~k − ~k ′)
|~Q| = 2k sin θ =4π
λsin θ
The scattering from the second electron willhave a phase shift of φ = ~Q ·~r .
A(~Q) = −r0(
1 + e i ~Q·~r)
I (~Q) = A(~Q)∗A(~Q)
= r20
(1 + e i ~Q·~r
)(1 + e−i ~Q·~r
)I (~Q) = r20
(1 + e i ~Q·~r + e−i ~Q·~r + 1
)= 2r20
(1 + cos(~Q ·~r)
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Scattering from many electrons
for many electrons
generalizing to a crystal
A(~Q) = −r0∑
j
e i ~Q·~rj
A(~Q) = −r0∑
N
e i ~Q· ~RN∑
j
e i ~Q·~rj
Since experiments measure I ∝ A2, the phase information is lost. This is aproblem if we don’t know the specific orientation of the scattering systemrelative to the x-ray beam.
We will now look at the consequences of this orientation and generalize tomore than two electrons
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 20 / 23
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Scattering from many electrons
for many electrons
generalizing to a crystal
A(~Q) = −r0∑
j
e i ~Q·~rj
A(~Q) = −r0∑
N
e i ~Q· ~RN∑
j
e i ~Q·~rj
Since experiments measure I ∝ A2, the phase information is lost. This is aproblem if we don’t know the specific orientation of the scattering systemrelative to the x-ray beam.
We will now look at the consequences of this orientation and generalize tomore than two electrons
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 20 / 23
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Scattering from many electrons
for many electrons
generalizing to a crystal
A(~Q) = −r0∑
j
e i ~Q·~rj
A(~Q) = −r0∑
N
e i ~Q· ~RN∑
j
e i ~Q·~rj
Since experiments measure I ∝ A2, the phase information is lost. This is aproblem if we don’t know the specific orientation of the scattering systemrelative to the x-ray beam.
We will now look at the consequences of this orientation and generalize tomore than two electrons
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 20 / 23
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Scattering from many electrons
for many electrons
generalizing to a crystal
A(~Q) = −r0∑
j
e i ~Q·~rj
A(~Q) = −r0∑
N
e i ~Q· ~RN∑
j
e i ~Q·~rj
Since experiments measure I ∝ A2, the phase information is lost. This is aproblem if we don’t know the specific orientation of the scattering systemrelative to the x-ray beam.
We will now look at the consequences of this orientation and generalize tomore than two electrons
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 20 / 23
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Scattering from many electrons
for many electrons
generalizing to a crystal
A(~Q) = −r0∑
j
e i ~Q·~rj
A(~Q) = −r0∑
N
e i ~Q· ~RN∑
j
e i ~Q·~rj
Since experiments measure I ∝ A2, the phase information is lost. This is aproblem if we don’t know the specific orientation of the scattering systemrelative to the x-ray beam.
We will now look at the consequences of this orientation and generalize tomore than two electrons
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 20 / 23
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Scattering from many electrons
for many electrons
generalizing to a crystal
A(~Q) = −r0∑
j
e i ~Q·~rj
A(~Q) = −r0∑
N
e i ~Q· ~RN∑
j
e i ~Q·~rj
Since experiments measure I ∝ A2, the phase information is lost. This is aproblem if we don’t know the specific orientation of the scattering systemrelative to the x-ray beam.
We will now look at the consequences of this orientation and generalize tomore than two electrons
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 20 / 23
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Two electrons — fixed orientation
The expression
I (~Q) = 2r20
(1 + cos(~Q ·~r)
)assumes that the two electronshave a specific, fixed orienta-tion. In this case the intensityas a function of Q is.
Fixed orientation is not theusual case, particularly for solu-tion and small-angle scattering. 0 0.5 1 1.5 2
Q (units of 2π/r)
0
1
2
3
4
Inte
nsity (
units o
f r2 o
)
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Two electrons — fixed orientation
The expression
I (~Q) = 2r20
(1 + cos(~Q ·~r)
)assumes that the two electronshave a specific, fixed orienta-tion. In this case the intensityas a function of Q is.
Fixed orientation is not theusual case, particularly for solu-tion and small-angle scattering.
0 0.5 1 1.5 2
Q (units of 2π/r)
0
1
2
3
4
Inte
nsity (
units o
f r2 o
)
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 21 / 23
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Two electrons — fixed orientation
The expression
I (~Q) = 2r20
(1 + cos(~Q ·~r)
)assumes that the two electronshave a specific, fixed orienta-tion. In this case the intensityas a function of Q is.
Fixed orientation is not theusual case, particularly for solu-tion and small-angle scattering. 0 0.5 1 1.5 2
Q (units of 2π/r)
0
1
2
3
4
Inte
nsity (
units o
f r2 o
)
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 21 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 22 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 22 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r
⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 22 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r
⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in space
and we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 22 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩
⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in space
and we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 22 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩
⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 22 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 22 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 22 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ
⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 22 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ
⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 22 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr
=sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ
⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ
⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 22 / 23
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Orientation averaging
A(~Q) = f1 + f2ei ~Q·~r
I (~Q) = f 21 + f 22 + f1f2ei ~Q·~r + f1f2e
−i ~Q·~r⟨I (~Q)
⟩= f 21 + f 22 + 2f1f2
⟨e i ~Q·~r
⟩⟨e i ~Q·~r
⟩=
∫e iQr cos θ sin θdθdφ∫
sin θdθdφ
=1
4π2π
∫ π
0e iQr cos θ sin θdθ
=2π
4π
(− 1
iQr
)∫ −iQr
iQrexdx
=1
22
sin(Qr)
Qr=
sin(Qr)
Qr
Consider scattering from twoarbitrary electron distribu-tions, f1 and f2. A(~Q), isgiven by
and the intensity, I (~Q), is
if the distance between thescatterers,~r , remains constant(no vibrations) but is allowedto orient randomly in spaceand we take ~Q along the z-axis
substituting x = iQr cos θ anddx = −iQr sin θdθ⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
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Randomly oriented electrons
⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
Recall that when we had a fixedorientation of the two electrons,we had and intensity variationI (~Q) = 2r20 (1 + cos(Qr)).
When we now replace the twoarbitrary scattering distributionswith electrons (f1, f2 → −r0),we change the intensity profilesignificantly.⟨I (~Q)
⟩= 2r20
(1 +
sin(Qr)
Qr
)0 0.5 1 1.5 2
Q (units of 2π/r)
0
1
2
3
4
Inte
nsity (
units o
f r2 o
)
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Randomly oriented electrons
⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
Recall that when we had a fixedorientation of the two electrons,we had and intensity variationI (~Q) = 2r20 (1 + cos(Qr)).
When we now replace the twoarbitrary scattering distributionswith electrons (f1, f2 → −r0),we change the intensity profilesignificantly.⟨I (~Q)
⟩= 2r20
(1 +
sin(Qr)
Qr
)0 0.5 1 1.5 2
Q (units of 2π/r)
0
1
2
3
4
Inte
nsity (
units o
f r2 o
)
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 23 / 23
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Randomly oriented electrons
⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
Recall that when we had a fixedorientation of the two electrons,we had and intensity variationI (~Q) = 2r20 (1 + cos(Qr)).
When we now replace the twoarbitrary scattering distributionswith electrons (f1, f2 → −r0),we change the intensity profilesignificantly.⟨I (~Q)
⟩= 2r20
(1 +
sin(Qr)
Qr
)
0 0.5 1 1.5 2
Q (units of 2π/r)
0
1
2
3
4
Inte
nsity (
units o
f r2 o
)
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 23 / 23
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Randomly oriented electrons
⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
Recall that when we had a fixedorientation of the two electrons,we had and intensity variationI (~Q) = 2r20 (1 + cos(Qr)).
When we now replace the twoarbitrary scattering distributionswith electrons (f1, f2 → −r0),we change the intensity profilesignificantly.
⟨I (~Q)
⟩= 2r20
(1 +
sin(Qr)
Qr
)
0 0.5 1 1.5 2
Q (units of 2π/r)
0
1
2
3
4
Inte
nsity (
units o
f r2 o
)
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 23 / 23
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Randomly oriented electrons
⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
Recall that when we had a fixedorientation of the two electrons,we had and intensity variationI (~Q) = 2r20 (1 + cos(Qr)).
When we now replace the twoarbitrary scattering distributionswith electrons (f1, f2 → −r0),we change the intensity profilesignificantly.⟨I (~Q)
⟩= 2r20
(1 +
sin(Qr)
Qr
)0 0.5 1 1.5 2
Q (units of 2π/r)
0
1
2
3
4
Inte
nsity (
units o
f r2 o
)
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 23 / 23
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Randomly oriented electrons
⟨I (~Q)
⟩= f 21 +f 22 +2f1f2
sin(Qr)
Qr
Recall that when we had a fixedorientation of the two electrons,we had and intensity variationI (~Q) = 2r20 (1 + cos(Qr)).
When we now replace the twoarbitrary scattering distributionswith electrons (f1, f2 → −r0),we change the intensity profilesignificantly.⟨I (~Q)
⟩= 2r20
(1 +
sin(Qr)
Qr
)0 0.5 1 1.5 2
Q (units of 2π/r)
0
1
2
3
4
Inte
nsity (
units o
f r2 o
)
C. Segre (IIT) PHYS 570 - Spring 2018 February 13, 2018 23 / 23