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Today’s Outline - November 14, 2016
• Kramers-Kronig relations
• Friedel’s Law
• Bijvoet (Bay-voot) Pairs
• MAD Phasing
• Quantum Origin of Resonant Scattering
• Imaging
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change) 16:00-18:00
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 1 / 19
Today’s Outline - November 14, 2016
• Kramers-Kronig relations
• Friedel’s Law
• Bijvoet (Bay-voot) Pairs
• MAD Phasing
• Quantum Origin of Resonant Scattering
• Imaging
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change) 16:00-18:00
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 1 / 19
Today’s Outline - November 14, 2016
• Kramers-Kronig relations
• Friedel’s Law
• Bijvoet (Bay-voot) Pairs
• MAD Phasing
• Quantum Origin of Resonant Scattering
• Imaging
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change) 16:00-18:00
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 1 / 19
Today’s Outline - November 14, 2016
• Kramers-Kronig relations
• Friedel’s Law
• Bijvoet (Bay-voot) Pairs
• MAD Phasing
• Quantum Origin of Resonant Scattering
• Imaging
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change) 16:00-18:00
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 1 / 19
Today’s Outline - November 14, 2016
• Kramers-Kronig relations
• Friedel’s Law
• Bijvoet (Bay-voot) Pairs
• MAD Phasing
• Quantum Origin of Resonant Scattering
• Imaging
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change) 16:00-18:00
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 1 / 19
Today’s Outline - November 14, 2016
• Kramers-Kronig relations
• Friedel’s Law
• Bijvoet (Bay-voot) Pairs
• MAD Phasing
• Quantum Origin of Resonant Scattering
• Imaging
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change) 16:00-18:00
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 1 / 19
Today’s Outline - November 14, 2016
• Kramers-Kronig relations
• Friedel’s Law
• Bijvoet (Bay-voot) Pairs
• MAD Phasing
• Quantum Origin of Resonant Scattering
• Imaging
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change) 16:00-18:00
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 1 / 19
Today’s Outline - November 14, 2016
• Kramers-Kronig relations
• Friedel’s Law
• Bijvoet (Bay-voot) Pairs
• MAD Phasing
• Quantum Origin of Resonant Scattering
• Imaging
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change) 16:00-18:00
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 1 / 19
Today’s Outline - November 14, 2016
• Kramers-Kronig relations
• Friedel’s Law
• Bijvoet (Bay-voot) Pairs
• MAD Phasing
• Quantum Origin of Resonant Scattering
• Imaging
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change) 16:00-18:00
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 1 / 19
Today’s Outline - November 14, 2016
• Kramers-Kronig relations
• Friedel’s Law
• Bijvoet (Bay-voot) Pairs
• MAD Phasing
• Quantum Origin of Resonant Scattering
• Imaging
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change) 16:00-18:00
Provide me with the paper you intend to present and a preferred sessionfor the exam
Send me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 1 / 19
Today’s Outline - November 14, 2016
• Kramers-Kronig relations
• Friedel’s Law
• Bijvoet (Bay-voot) Pairs
• MAD Phasing
• Quantum Origin of Resonant Scattering
• Imaging
Homework Assignment #7:Chapter 7: 2,3,9,10,11due Monday, November 28, 2016
Final Exam, Wednesday, December 7, 2016, Stuart Building 2132 sessions: 09:00-12:00; 13:00-17:00; (this may change) 16:00-18:00
Provide me with the paper you intend to present and a preferred sessionfor the examSend me your presentation in Powerpoint or PDF format before beforeyour session
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 1 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter.
Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial, whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t) = −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial, whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t) = −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial,
whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t) = −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial,
whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t)
= (ε− ε0)~E (t) = −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial,
whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t)
= −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial, whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t)
= −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial, whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t)
= −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial, whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t) = −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial, whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t) = −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial, whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t) = −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0
=
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial, whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t) = −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial, whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t) = −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2
=ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
Scattering and refraction are alternative ways to approach the phenomenonof x-ray interaction with matter. Thus the resonant response we have seenin scattering must be manifested in the index of refraction as well.
the electric field from the x-rays, ~E (t), induces a polar-ization response, ~P(t), in thematerial, whereχ = (ε/ε0 − 1)is the electric susceptibility
given an electron density ρand using the displacementfunction for the electrons inthe forced oscillator model
index of refraction can thusbe computed
~P(t) = ε0χ~E (t) = (ε− ε0)~E (t) = −eρx(t)
= −eρ(− e
m
) E0e−iωt
(ω2s − ω2 − iωΓ)
P(t)
E (t)= ε− ε0 =
(e2ρ
m
)1
(ω2s − ω2 − iωΓ)
n2 =c2
v2=
ε
ε0
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 2 / 19
Refractive index
n2 = 1 +
(e2ρ
ε0m
)1
(ω2s − ω2 − iωΓ)
= 1 +
(e2ρ
ε0m
)ω2s − ω2
(ω2s − ω2)2 + (ωΓ)2
+ iωΓ
(ω2s − ω2)2 + (ωΓ)2
-0.5
0
0.5
1
1.5
2
2.5
3
0.1 1 10
Re
[n2]
ω/ωs
0
0.5
1
1.5
2
2.5
3
0.1 1 10
Im[n
2]
ω/ωs
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 3 / 19
Refractive index
n2 = 1 +
(e2ρ
ε0m
)1
(ω2s − ω2 − iωΓ)
= 1 +
(e2ρ
ε0m
)ω2s − ω2
(ω2s − ω2)2 + (ωΓ)2
+ iωΓ
(ω2s − ω2)2 + (ωΓ)2
-0.5
0
0.5
1
1.5
2
2.5
3
0.1 1 10
Re
[n2]
ω/ωs
0
0.5
1
1.5
2
2.5
3
0.1 1 10
Im[n
2]
ω/ωs
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 3 / 19
Refractive index
n2 = 1 +
(e2ρ
ε0m
)1
(ω2s − ω2 − iωΓ)
= 1 +
(e2ρ
ε0m
)ω2s − ω2
(ω2s − ω2)2 + (ωΓ)2
+ iωΓ
(ω2s − ω2)2 + (ωΓ)2
-0.5
0
0.5
1
1.5
2
2.5
3
0.1 1 10
Re
[n2]
ω/ωs
0
0.5
1
1.5
2
2.5
3
0.1 1 10
Im[n
2]
ω/ωs
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 3 / 19
Absorption cross-section
Electrons in atoms are bound andtherefore have resonant effects dueto the binding forces
the imaginary part of the resonantscattering for an electron bound toan atom shows a frequency depen-dence with a peak at ω ≈ ωs
this single oscillator model, how-ever, does not reproduce theobserved absorption cross-sectionjump at an absorption edge
f ′′s (ω) =ω2sωΓ
(ω2 − ω2s )2 + (ωΓ)2
r20
0
0.2
0.4
0.6
0.8
1
1.2
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
,s
ω/ωs
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 4 / 19
Absorption cross-section
Electrons in atoms are bound andtherefore have resonant effects dueto the binding forces
the imaginary part of the resonantscattering for an electron bound toan atom shows a frequency depen-dence with a peak at ω ≈ ωs
this single oscillator model, how-ever, does not reproduce theobserved absorption cross-sectionjump at an absorption edge
f ′′s (ω) =ω2sωΓ
(ω2 − ω2s )2 + (ωΓ)2
r20
0
0.2
0.4
0.6
0.8
1
1.2
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
,s
ω/ωs
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 4 / 19
Absorption cross-section
Electrons in atoms are bound andtherefore have resonant effects dueto the binding forces
the imaginary part of the resonantscattering for an electron bound toan atom shows a frequency depen-dence with a peak at ω ≈ ωs
this single oscillator model, how-ever, does not reproduce theobserved absorption cross-sectionjump at an absorption edge
f ′′s (ω) =ω2sωΓ
(ω2 − ω2s )2 + (ωΓ)2
r20
0
0.2
0.4
0.6
0.8
1
1.2
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
,s
ω/ωs
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 4 / 19
Absorption cross-section
Electrons in atoms are bound andtherefore have resonant effects dueto the binding forces
the imaginary part of the resonantscattering for an electron bound toan atom shows a frequency depen-dence with a peak at ω ≈ ωs
this single oscillator model, how-ever, does not reproduce theobserved absorption cross-sectionjump at an absorption edge
f ′′s (ω) =ω2sωΓ
(ω2 − ω2s )2 + (ωΓ)2
r20
0
0.2
0.4
0.6
0.8
1
1.2
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
,s
ω/ωs
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 4 / 19
Absorption cross-section
Electrons in atoms are bound andtherefore have resonant effects dueto the binding forces
the imaginary part of the resonantscattering for an electron bound toan atom shows a frequency depen-dence with a peak at ω ≈ ωs
this single oscillator model, how-ever, does not reproduce theobserved absorption cross-sectionjump at an absorption edge
f ′′s (ω) =ω2sωΓ
(ω2 − ω2s )2 + (ωΓ)2
r20
0
0.2
0.4
0.6
0.8
1
1.2
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
,s
ω/ωs
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 4 / 19
Absorption cross-section
Electrons in atoms are bound andtherefore have resonant effects dueto the binding forces
the imaginary part of the resonantscattering for an electron bound toan atom shows a frequency depen-dence with a peak at ω ≈ ωs
this single oscillator model, how-ever, does not reproduce theobserved absorption cross-sectionjump at an absorption edge
f ′′s (ω) =ω2sωΓ
(ω2 − ω2s )2 + (ωΓ)2
r20
0
0.2
0.4
0.6
0.8
1
1.2
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
,s
ω/ωs
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 4 / 19
Multi-oscillator model
The damping constant, Γis gener-ally much less than the resonantfrequency, ωs
thus the single oscillator is essen-tially a delta function
in a real atom, exceeding the ab-sorption edge allows the electronto be excited into a continuum ofstates which can be approximatedby a sum of resonant oscillatorswith frequency distribution g(ωs)
σa(ω) = 2π2r0c∑s
g(ωs)δ(ω − ωs)
a similar effect is seen in the reso-nant scattering term f ′(w)
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
≈4πr0cπ
2δ(ω − ωs)
0
0.5
1
1.5
2
2.5
3
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
ω/ωs
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 5 / 19
Multi-oscillator model
The damping constant, Γis gener-ally much less than the resonantfrequency, ωs
thus the single oscillator is essen-tially a delta function
in a real atom, exceeding the ab-sorption edge allows the electronto be excited into a continuum ofstates which can be approximatedby a sum of resonant oscillatorswith frequency distribution g(ωs)
σa(ω) = 2π2r0c∑s
g(ωs)δ(ω − ωs)
a similar effect is seen in the reso-nant scattering term f ′(w)
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
≈4πr0cπ
2δ(ω − ωs)
0
0.5
1
1.5
2
2.5
3
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
ω/ωs
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 5 / 19
Multi-oscillator model
The damping constant, Γis gener-ally much less than the resonantfrequency, ωs
thus the single oscillator is essen-tially a delta function
in a real atom, exceeding the ab-sorption edge allows the electronto be excited into a continuum ofstates which can be approximatedby a sum of resonant oscillatorswith frequency distribution g(ωs)
σa(ω) = 2π2r0c∑s
g(ωs)δ(ω − ωs)
a similar effect is seen in the reso-nant scattering term f ′(w)
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
≈4πr0cπ
2δ(ω − ωs)
0
0.5
1
1.5
2
2.5
3
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
ω/ωs
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 5 / 19
Multi-oscillator model
The damping constant, Γis gener-ally much less than the resonantfrequency, ωs
thus the single oscillator is essen-tially a delta function
in a real atom, exceeding the ab-sorption edge allows the electronto be excited into a continuum ofstates which can be approximatedby a sum of resonant oscillatorswith frequency distribution g(ωs)
σa(ω) = 2π2r0c∑s
g(ωs)δ(ω − ωs)
a similar effect is seen in the reso-nant scattering term f ′(w)
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
≈4πr0cπ
2δ(ω − ωs)
0
0.5
1
1.5
2
2.5
3
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
ω/ωs
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 5 / 19
Multi-oscillator model
The damping constant, Γis gener-ally much less than the resonantfrequency, ωs
thus the single oscillator is essen-tially a delta function
in a real atom, exceeding the ab-sorption edge allows the electronto be excited into a continuum ofstates which can be approximatedby a sum of resonant oscillatorswith frequency distribution g(ωs)
σa(ω) = 2π2r0c∑s
g(ωs)δ(ω − ωs)
a similar effect is seen in the reso-nant scattering term f ′(w)
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
≈4πr0cπ
2δ(ω − ωs)
0
0.5
1
1.5
2
2.5
3
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
ω/ωs
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 5 / 19
Multi-oscillator model
The damping constant, Γis gener-ally much less than the resonantfrequency, ωs
thus the single oscillator is essen-tially a delta function
in a real atom, exceeding the ab-sorption edge allows the electronto be excited into a continuum ofstates which can be approximatedby a sum of resonant oscillatorswith frequency distribution g(ωs)
σa(ω) = 2π2r0c∑s
g(ωs)δ(ω − ωs)
a similar effect is seen in the reso-nant scattering term f ′(w)
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
≈4πr0cπ
2δ(ω − ωs)
0
0.5
1
1.5
2
2.5
3
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
ω/ωs
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 5 / 19
Multi-oscillator model
The damping constant, Γis gener-ally much less than the resonantfrequency, ωs
thus the single oscillator is essen-tially a delta function
in a real atom, exceeding the ab-sorption edge allows the electronto be excited into a continuum ofstates which can be approximatedby a sum of resonant oscillatorswith frequency distribution g(ωs)
σa(ω) = 2π2r0c∑s
g(ωs)δ(ω − ωs)
a similar effect is seen in the reso-nant scattering term f ′(w)
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
≈4πr0cπ
2δ(ω − ωs)
0
0.5
1
1.5
2
2.5
3
0.6 0.8 1 1.2 1.4 1.6 1.8 2
σa
ω/ωs
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 5 / 19
Multi-oscillator model
The damping constant, Γis gener-ally much less than the resonantfrequency, ωs
thus the single oscillator is essen-tially a delta function
in a real atom, exceeding the ab-sorption edge allows the electronto be excited into a continuum ofstates which can be approximatedby a sum of resonant oscillatorswith frequency distribution g(ωs)
σa(ω) = 2π2r0c∑s
g(ωs)δ(ω − ωs)
a similar effect is seen in the reso-nant scattering term f ′(w)
σa,s(ω) = 4πr0cω2s Γ
(ω2 − ω2s )2 + (ωΓ)2
≈4πr0cπ
2δ(ω − ωs)
-0.1
-0.08
-0.06
-0.04
-0.02
0
0.02
0.04
0.06
0.6 0.8 1 1.2 1.4 1.6 1.8 2
f’
ω/ωs
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 5 / 19
Kramers-Kronig relations
It is generally not a good idea to rely on theoretical calculations of thedispersion corrections.
However, if it is possible to obtain the experimentalabsorption cross-section, σa, the resonant scattering can be computed.
first compute f ′′(ω) from themeasured absorption cross-section
f ′′(ω) = −(
ω
4πr0c
)σa(ω)
then use the Kramers-Kronig relations which connect the resonant term tothe absorptive term and where all the integrals are “principal value”integrals
f ′(ω) =1
πP∫ +∞
−∞
f ′′(ω′)
(ω′ − ω)dω′ =
2
πP∫ +∞
0
ω′f ′′(ω′)
(ω′2 − ω2)dω′
f ′′(ω) = − 1
πP∫ +∞
−∞
f ′(ω′)
(ω′ − ω)dω′ = −2ω
πP∫ +∞
0
f ′(ω′)
(ω′2 − ω2)dω′
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 6 / 19
Kramers-Kronig relations
It is generally not a good idea to rely on theoretical calculations of thedispersion corrections. However, if it is possible to obtain the experimentalabsorption cross-section, σa, the resonant scattering can be computed.
first compute f ′′(ω) from themeasured absorption cross-section
f ′′(ω) = −(
ω
4πr0c
)σa(ω)
then use the Kramers-Kronig relations which connect the resonant term tothe absorptive term and where all the integrals are “principal value”integrals
f ′(ω) =1
πP∫ +∞
−∞
f ′′(ω′)
(ω′ − ω)dω′ =
2
πP∫ +∞
0
ω′f ′′(ω′)
(ω′2 − ω2)dω′
f ′′(ω) = − 1
πP∫ +∞
−∞
f ′(ω′)
(ω′ − ω)dω′ = −2ω
πP∫ +∞
0
f ′(ω′)
(ω′2 − ω2)dω′
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 6 / 19
Kramers-Kronig relations
It is generally not a good idea to rely on theoretical calculations of thedispersion corrections. However, if it is possible to obtain the experimentalabsorption cross-section, σa, the resonant scattering can be computed.
first compute f ′′(ω) from themeasured absorption cross-section
f ′′(ω) = −(
ω
4πr0c
)σa(ω)
then use the Kramers-Kronig relations which connect the resonant term tothe absorptive term and where all the integrals are “principal value”integrals
f ′(ω) =1
πP∫ +∞
−∞
f ′′(ω′)
(ω′ − ω)dω′ =
2
πP∫ +∞
0
ω′f ′′(ω′)
(ω′2 − ω2)dω′
f ′′(ω) = − 1
πP∫ +∞
−∞
f ′(ω′)
(ω′ − ω)dω′ = −2ω
πP∫ +∞
0
f ′(ω′)
(ω′2 − ω2)dω′
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 6 / 19
Kramers-Kronig relations
It is generally not a good idea to rely on theoretical calculations of thedispersion corrections. However, if it is possible to obtain the experimentalabsorption cross-section, σa, the resonant scattering can be computed.
first compute f ′′(ω) from themeasured absorption cross-section
f ′′(ω) = −(
ω
4πr0c
)σa(ω)
then use the Kramers-Kronig relations which connect the resonant term tothe absorptive term and where all the integrals are “principal value”integrals
f ′(ω) =1
πP∫ +∞
−∞
f ′′(ω′)
(ω′ − ω)dω′ =
2
πP∫ +∞
0
ω′f ′′(ω′)
(ω′2 − ω2)dω′
f ′′(ω) = − 1
πP∫ +∞
−∞
f ′(ω′)
(ω′ − ω)dω′ = −2ω
πP∫ +∞
0
f ′(ω′)
(ω′2 − ω2)dω′
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 6 / 19
Kramers-Kronig relations
It is generally not a good idea to rely on theoretical calculations of thedispersion corrections. However, if it is possible to obtain the experimentalabsorption cross-section, σa, the resonant scattering can be computed.
first compute f ′′(ω) from themeasured absorption cross-section
f ′′(ω) = −(
ω
4πr0c
)σa(ω)
then use the Kramers-Kronig relations which connect the resonant term tothe absorptive term
and where all the integrals are “principal value”integrals
f ′(ω) =1
πP∫ +∞
−∞
f ′′(ω′)
(ω′ − ω)dω′ =
2
πP∫ +∞
0
ω′f ′′(ω′)
(ω′2 − ω2)dω′
f ′′(ω) = − 1
πP∫ +∞
−∞
f ′(ω′)
(ω′ − ω)dω′ = −2ω
πP∫ +∞
0
f ′(ω′)
(ω′2 − ω2)dω′
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 6 / 19
Kramers-Kronig relations
It is generally not a good idea to rely on theoretical calculations of thedispersion corrections. However, if it is possible to obtain the experimentalabsorption cross-section, σa, the resonant scattering can be computed.
first compute f ′′(ω) from themeasured absorption cross-section
f ′′(ω) = −(
ω
4πr0c
)σa(ω)
then use the Kramers-Kronig relations which connect the resonant term tothe absorptive term
and where all the integrals are “principal value”integrals
f ′(ω) =1
πP∫ +∞
−∞
f ′′(ω′)
(ω′ − ω)dω′
=2
πP∫ +∞
0
ω′f ′′(ω′)
(ω′2 − ω2)dω′
f ′′(ω) = − 1
πP∫ +∞
−∞
f ′(ω′)
(ω′ − ω)dω′ = −2ω
πP∫ +∞
0
f ′(ω′)
(ω′2 − ω2)dω′
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 6 / 19
Kramers-Kronig relations
It is generally not a good idea to rely on theoretical calculations of thedispersion corrections. However, if it is possible to obtain the experimentalabsorption cross-section, σa, the resonant scattering can be computed.
first compute f ′′(ω) from themeasured absorption cross-section
f ′′(ω) = −(
ω
4πr0c
)σa(ω)
then use the Kramers-Kronig relations which connect the resonant term tothe absorptive term
and where all the integrals are “principal value”integrals
f ′(ω) =1
πP∫ +∞
−∞
f ′′(ω′)
(ω′ − ω)dω′
=2
πP∫ +∞
0
ω′f ′′(ω′)
(ω′2 − ω2)dω′
f ′′(ω) = − 1
πP∫ +∞
−∞
f ′(ω′)
(ω′ − ω)dω′
= −2ω
πP∫ +∞
0
f ′(ω′)
(ω′2 − ω2)dω′
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 6 / 19
Kramers-Kronig relations
It is generally not a good idea to rely on theoretical calculations of thedispersion corrections. However, if it is possible to obtain the experimentalabsorption cross-section, σa, the resonant scattering can be computed.
first compute f ′′(ω) from themeasured absorption cross-section
f ′′(ω) = −(
ω
4πr0c
)σa(ω)
then use the Kramers-Kronig relations which connect the resonant term tothe absorptive term
and where all the integrals are “principal value”integrals
f ′(ω) =1
πP∫ +∞
−∞
f ′′(ω′)
(ω′ − ω)dω′ =
2
πP∫ +∞
0
ω′f ′′(ω′)
(ω′2 − ω2)dω′
f ′′(ω) = − 1
πP∫ +∞
−∞
f ′(ω′)
(ω′ − ω)dω′
= −2ω
πP∫ +∞
0
f ′(ω′)
(ω′2 − ω2)dω′
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 6 / 19
Kramers-Kronig relations
It is generally not a good idea to rely on theoretical calculations of thedispersion corrections. However, if it is possible to obtain the experimentalabsorption cross-section, σa, the resonant scattering can be computed.
first compute f ′′(ω) from themeasured absorption cross-section
f ′′(ω) = −(
ω
4πr0c
)σa(ω)
then use the Kramers-Kronig relations which connect the resonant term tothe absorptive term
and where all the integrals are “principal value”integrals
f ′(ω) =1
πP∫ +∞
−∞
f ′′(ω′)
(ω′ − ω)dω′ =
2
πP∫ +∞
0
ω′f ′′(ω′)
(ω′2 − ω2)dω′
f ′′(ω) = − 1
πP∫ +∞
−∞
f ′(ω′)
(ω′ − ω)dω′ = −2ω
πP∫ +∞
0
f ′(ω′)
(ω′2 − ω2)dω′
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 6 / 19
Kramers-Kronig relations
It is generally not a good idea to rely on theoretical calculations of thedispersion corrections. However, if it is possible to obtain the experimentalabsorption cross-section, σa, the resonant scattering can be computed.
first compute f ′′(ω) from themeasured absorption cross-section
f ′′(ω) = −(
ω
4πr0c
)σa(ω)
then use the Kramers-Kronig relations which connect the resonant term tothe absorptive term and where all the integrals are “principal value”integrals
f ′(ω) =1
πP∫ +∞
−∞
f ′′(ω′)
(ω′ − ω)dω′ =
2
πP∫ +∞
0
ω′f ′′(ω′)
(ω′2 − ω2)dω′
f ′′(ω) = − 1
πP∫ +∞
−∞
f ′(ω′)
(ω′ − ω)dω′ = −2ω
πP∫ +∞
0
f ′(ω′)
(ω′2 − ω2)dω′
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 6 / 19
Calculated cross-sections
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 7 / 19
Calculated cross-sections
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 7 / 19
Scattering from two unlike atoms
Two unlike atoms with scatter-ing factors f1 and f2 are orientedby a vector pointing from thelarger to the smaller.
Consider two cases, with thescattering vector Q in the samedirection as the orientation vec-tor and opposite to the orienta-tion vector.
Now compute the scattered in-tensity in each case, assumingscattering factors are purely real.
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 8 / 19
Scattering from two unlike atoms
Two unlike atoms with scatter-ing factors f1 and f2 are orientedby a vector pointing from thelarger to the smaller.
Consider two cases, with thescattering vector Q
in the samedirection as the orientation vec-tor and opposite to the orienta-tion vector.
Now compute the scattered in-tensity in each case, assumingscattering factors are purely real.
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 8 / 19
Scattering from two unlike atoms
Two unlike atoms with scatter-ing factors f1 and f2 are orientedby a vector pointing from thelarger to the smaller.
Consider two cases, with thescattering vector Q in the samedirection as the orientation vec-tor
and opposite to the orienta-tion vector.
Now compute the scattered in-tensity in each case, assumingscattering factors are purely real.
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 8 / 19
Scattering from two unlike atoms
Two unlike atoms with scatter-ing factors f1 and f2 are orientedby a vector pointing from thelarger to the smaller.
Consider two cases, with thescattering vector Q in the samedirection as the orientation vec-tor and opposite to the orienta-tion vector.
Now compute the scattered in-tensity in each case, assumingscattering factors are purely real.
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 8 / 19
Scattering from two unlike atoms
Two unlike atoms with scatter-ing factors f1 and f2 are orientedby a vector pointing from thelarger to the smaller.
Consider two cases, with thescattering vector Q in the samedirection as the orientation vec-tor and opposite to the orienta-tion vector.
Now compute the scattered in-tensity in each case, assumingscattering factors are purely real.
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 8 / 19
Friedel’s Law
A(+Q) = f1 + f2e+iQx
I (+Q) = (f1 + f2e+iQx)(f1 + f2e
−iQx)
= f 21 + f 22 + 2f1f2 cos(Qx)
I (+Q) = I (−Q) Friedel′s Law
A(−Q) = f1 + f2e−iQx
I (−Q) = (f1 + f2e−iQx)(f1 + f2e
+iQx)
= f 21 + f 22 + 2f1f2 cos(Qx)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 9 / 19
Friedel’s Law
A(+Q) = f1 + f2e+iQx
I (+Q) = (f1 + f2e+iQx)(f1 + f2e
−iQx)
= f 21 + f 22 + 2f1f2 cos(Qx)
I (+Q) = I (−Q) Friedel′s Law
A(−Q) = f1 + f2e−iQx
I (−Q) = (f1 + f2e−iQx)(f1 + f2e
+iQx)
= f 21 + f 22 + 2f1f2 cos(Qx)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 9 / 19
Friedel’s Law
A(+Q) = f1 + f2e+iQx
I (+Q) = (f1 + f2e+iQx)(f1 + f2e
−iQx)
= f 21 + f 22 + 2f1f2 cos(Qx)
I (+Q) = I (−Q) Friedel′s Law
A(−Q) = f1 + f2e−iQx
I (−Q) = (f1 + f2e−iQx)(f1 + f2e
+iQx)
= f 21 + f 22 + 2f1f2 cos(Qx)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 9 / 19
Friedel’s Law
A(+Q) = f1 + f2e+iQx
I (+Q) = (f1 + f2e+iQx)(f1 + f2e
−iQx)
= f 21 + f 22 + 2f1f2 cos(Qx)
I (+Q) = I (−Q) Friedel′s Law
A(−Q) = f1 + f2e−iQx
I (−Q) = (f1 + f2e−iQx)(f1 + f2e
+iQx)
= f 21 + f 22 + 2f1f2 cos(Qx)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 9 / 19
Friedel’s Law
A(+Q) = f1 + f2e+iQx
I (+Q) = (f1 + f2e+iQx)(f1 + f2e
−iQx)
= f 21 + f 22 + 2f1f2 cos(Qx)
I (+Q) = I (−Q) Friedel′s Law
A(−Q) = f1 + f2e−iQx
I (−Q) = (f1 + f2e−iQx)(f1 + f2e
+iQx)
= f 21 + f 22 + 2f1f2 cos(Qx)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 9 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j
= rjeiφj
j = 1, 2 rj = |fj |A(Q) = r1e
iφ1 + r2eiφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j
= rjeiφj
j = 1, 2
rj = |fj |A(Q) = r1e
iφ1 + r2eiφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j = rjeiφj j = 1, 2 rj = |fj |
A(Q) = r1eiφ1 + r2e
iφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j = rjeiφj j = 1, 2 rj = |fj |
A(Q) = r1eiφ1 + r2e
iφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j = rjeiφj j = 1, 2 rj = |fj |
A(Q) = r1eiφ1 + r2e
iφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j = rjeiφj j = 1, 2 rj = |fj |
A(Q) = r1eiφ1 + r2e
iφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j = rjeiφj j = 1, 2 rj = |fj |
A(Q) = r1eiφ1 + r2e
iφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j = rjeiφj j = 1, 2 rj = |fj |
A(Q) = r1eiφ1 + r2e
iφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2)
6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j = rjeiφj j = 1, 2 rj = |fj |
A(Q) = r1eiφ1 + r2e
iφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j = rjeiφj j = 1, 2 rj = |fj |
A(Q) = r1eiφ1 + r2e
iφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j = rjeiφj j = 1, 2 rj = |fj |
A(Q) = r1eiφ1 + r2e
iφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j = rjeiφj j = 1, 2 rj = |fj |
A(Q) = r1eiφ1 + r2e
iφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Breakdown of Friedel’s Law
If the scattering factor has resonant terms which are not negligible, wehave to include them in the computation
fj = f 0j + f ′j + if ′′j = rjeiφj j = 1, 2 rj = |fj |
A(Q) = r1eiφ1 + r2e
iφ2e iQx
I (Q) = (r1eiφ1 + r2e
iφ2e iQx)(r1e−iφ1 + r2e
−iφ2e−iQx)
= r21 + r22 + r1r2eiφ1e−iφ2e−iQx + r1r2e
−iφ1e iφ2e iQx
= |f1|2 + |f2|2 + r1r2(e−(Qx+φ1−φ2) + e+(Qx+φ1−φ2))
I (Q) = |f1|2 + |f2|2 + 2r1r2 cos(Qx + φ1 − φ2) 6= I (−Q)
Thus, Friedel’s Law breaks down unless there is a center of symmetry:
F = r1e−i(φ1+Qx1) + r1e
−i(φ1−Qx1) + r2e−i(φ2+Qx2) + r2e
−i(φ2−Qx2)
= [2r1 cos(Qx1)]e−iφ1 + [2r2 cos(Qx2)]e−iφ2
I (Q) = 4|f1|2 + 4|f2|2 + 8|f1||f2| cos(Qx1) cos(Qx2) cos(φ2 − φ1)
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 10 / 19
Argand diagram
This can all be described graphically using an Argand diagram:
no resonant terms
including resonant terms
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 11 / 19
Argand diagram
This can all be described graphically using an Argand diagram:
no resonant terms including resonant terms
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 11 / 19
ZnS example
The ZnS structure is not cen-trosymmetric and when viewedalong the 〈111〉 direction, it showsalternating stacked planes of Znand S atoms.
Scattering from opposite faces of asingle crystal of ZnS gives a dif-ferent scattering factor and onecan deduce the terminating surfaceatom.
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 12 / 19
ZnS example
The ZnS structure is not cen-trosymmetric and when viewedalong the 〈111〉 direction, it showsalternating stacked planes of Znand S atoms.
Scattering from opposite faces of asingle crystal of ZnS gives a dif-ferent scattering factor and onecan deduce the terminating surfaceatom.
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 12 / 19
Bijvoet pairs - chiral molecules
Consider a tetrahedral molecule of carbon with four different species ateach corner, oriented so the lightest is projected to the origin.
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 13 / 19
Bijvoet pairs - chiral molecules
Consider a tetrahedral molecule of carbon with four different species ateach corner, oriented so the lightest is projected to the origin.
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 13 / 19
Atomic scattering factors
Each of the three atoms not at the origin has a scattering factor for ~Q asshown
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 14 / 19
Left handed scattering factor
FS = |fs |+ |fm|e−iφme iφ + |fl |e−iφl e−iφ
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 15 / 19
Left handed scattering factor
FS = |fs |+ |fm|e−iφme iφ + |fl |e−iφl e−iφ
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 15 / 19
Right handed scattering factor
FR = |fs |+ |fm|e−iφme−iφ + |fl |e−iφl e iφ
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 16 / 19
Right handed scattering factor
FR = |fs |+ |fm|e−iφme−iφ + |fl |e−iφl e iφ
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 16 / 19
Scattering factor comparison
It is thus possible to tell the difference in handedness of chiral moleculesimply by x-ray scattering
s
∣∣∣|fs |+ |fm|e−iφme iφ + |fl |e−iφl e−iφ∣∣∣2 6= ∣∣∣|fs |+ |fm|e−iφme−iφ + |fl |e−iφl e iφ
∣∣∣2
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 17 / 19
Scattering factor comparison
It is thus possible to tell the difference in handedness of chiral moleculesimply by x-ray scattering
s
∣∣∣|fs |+ |fm|e−iφme iφ + |fl |e−iφl e−iφ∣∣∣2 6= ∣∣∣|fs |+ |fm|e−iφme−iφ + |fl |e−iφl e iφ
∣∣∣2C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 17 / 19
MAD phasing
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 18 / 19
MAD phasing
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 18 / 19
MAD phasing
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 18 / 19
MAD phasing
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 18 / 19
Comparison of matrix elements
Absorption
e~A · ~pm
Thomson scattering
e2A2
2m
Resonant scattering
(e~A · ~pm
)2
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 19 / 19
Comparison of matrix elements
Absorption
e~A · ~pm
Thomson scattering
e2A2
2m
Resonant scattering
(e~A · ~pm
)2
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 19 / 19
Comparison of matrix elements
Absorption
e~A · ~pm
Thomson scattering
e2A2
2m
Resonant scattering
(e~A · ~pm
)2
C. Segre (IIT) PHYS 570 - Fall 2016 November 14, 2016 19 / 19