The scattering amplitude is a quantity of scattering theory that describes the directional dependence of the scattering wave when a plane wave is scattered at a scattering center. It has the dimension length and connects the S matrix with the cross section .
f
{\ displaystyle f}
definition
The scattering amplitude is defined by the S operator :
f
(
p
→
p
′
)
{\ displaystyle f (p \ to p ')}
S.
{\ displaystyle S}
⟨
p
′
|
S.
|
p
⟩
=
δ
(
3
)
(
p
→
′
-
p
→
)
+
i
2
π
m
δ
(
E.
′
-
E.
)
f
(
p
→
p
′
)
{\ displaystyle \ langle p '| S | p \ rangle = \ delta ^ {(3)} ({\ vec {p}}' - {\ vec {p}}) + {\ tfrac {\ mathrm {i} } {2 \ pi m}} \ delta (E'-E) f (p \ to p ')}
Are there
|
p
⟩
{\ displaystyle | p \ rangle}
the initial state and the final state with defined momentum , i.e. eigenstates of the momentum operator ,
|
p
′
⟩
{\ displaystyle | p '\ rangle}
p
→
,
p
→
′
{\ displaystyle {\ vec {p}}, {\ vec {p}} '}
the impulses of the states
E.
,
E.
′
{\ displaystyle E, E '}
the energy of the states
m
{\ displaystyle m}
the mass (physics) of the states and
δ
{\ displaystyle \ delta}
the Dirac distribution .
Alternative definition
An alternative representation is presented below, which is also often used as a definition. In it, the scattering amplitude can be written as a function of the energy of the incoming state as well as the angle between and , since the S operator and thus also the scattering amplitude are invariant under rotations :
θ
{\ displaystyle \ theta}
p
→
{\ displaystyle {\ vec {p}}}
p
→
′
{\ displaystyle {\ vec {p}} '}
ψ
O
u
t
(
p
→
′
)
=
⟨
p
′
|
ψ
O
u
t
⟩
=
⟨
p
′
|
S.
|
ψ
i
n
⟩
=
∫
d
3
p
→
⟨
p
′
|
S.
|
p
⟩
⟨
p
|
ψ
i
n
⟩
=
∫
d
3
p
→
⟨
p
′
|
S.
|
p
⟩
ψ
i
n
(
p
)
=
ψ
i
n
(
p
→
′
)
+
i
2
π
m
∫
d
3
p
→
δ
(
E.
′
-
E.
)
f
(
p
→
p
′
)
ψ
i
n
(
p
→
)
=
ψ
i
n
(
p
→
′
)
+
i
2
π
m
f
(
E.
′
,
θ
)
∫
d
3
p
→
δ
(
E.
′
-
E.
)
ψ
i
n
(
p
→
)
{\ displaystyle {\ begin {aligned} \ psi _ {\ mathrm {out}} ({\ vec {p}} ') & = \ langle p' | \ psi _ {\ mathrm {out}} \ rangle = \ langle p '| S | \ psi _ {\ mathrm {in}} \ rangle = \ int \ mathrm {d} ^ {3} {\ vec {p}} \, \ langle p' | S | p \ rangle \ langle p | \ psi _ {\ mathrm {in}} \ rangle = \ int \ mathrm {d} ^ {3} {\ vec {p}} \, \ langle p '| S | p \ rangle \, \ psi _ {\ mathrm {in}} (p) \\ & = \ psi _ {\ mathrm {in}} ({\ vec {p}} ') + {\ frac {\ mathrm {i}} {2 \ pi m}} \ int \ mathrm {d} ^ {3} {\ vec {p}} \, \ delta (E'-E) f (p \ to p ') \ psi _ {\ mathrm {in}} ( {\ vec {p}}) \\ & = \ psi _ {\ mathrm {in}} ({\ vec {p}} ') + {\ frac {\ mathrm {i}} {2 \ pi m}} f (E ', \ theta) \ int \ mathrm {d} ^ {3} {\ vec {p}} \, \ delta (E'-E) \; \ psi _ {\ mathrm {in}} ({ \ vec {p}}) \ end {aligned}}}
If a plane wave parallel to the z-axis is assumed for the incoming wave , this results in:
ψ
i
n
{\ displaystyle \ psi _ {\ mathrm {in}}}
ψ
O
u
t
(
p
′
)
=
e
i
p
′
z
+
f
(
E.
′
,
θ
)
e
i
p
′
r
r
{\ displaystyle \ psi _ {\ mathrm {out}} (p ') = e ^ {\ mathrm {i} p'z} + f (E', \ theta) \; {\ frac {e ^ {\ mathrm {i} p'r}} {r}}}
Cross section
The differential cross section is given by:
d
σ
d
Ω
=
|
f
(
ϑ
)
|
2
.
{\ displaystyle {\ frac {d \ sigma} {d \ Omega}} = | f (\ vartheta) | ^ {2} \ ;.}
For total cross section , there is a connection via the optical theorem :
σ
t
O
t
=
∫
4th
π
d
σ
d
Ω
⋅
d
Ω
=
4th
π
k
I.
m
f
(
0
)
{\ displaystyle \ sigma _ {\ mathrm {tot}} = \ int _ {4 \ pi} {\ frac {d \ sigma} {d \ Omega}} \ cdot d \ Omega = {\ frac {4 \ pi} {k}} ~ \ mathrm {Im} \, f (0)}
with the wave number and the imaginary part of the scattering amplitude for the scattering angle zero.
k
{\ displaystyle k}
I.
m
f
(
0
)
{\ displaystyle \ mathrm {Im} \, f (0)}
Partial wave development
In the partial wave expansion, the scattering amplitude is expressed as a sum over partial waves :
f
(
ϑ
)
=
∑
ℓ
=
0
∞
(
2
ℓ
+
1
)
f
ℓ
(
k
)
P
ℓ
(
cos
ϑ
)
{\ displaystyle f (\ vartheta) = \ sum _ {\ ell = 0} ^ {\ infty} (2 \ ell +1) \; f _ {\ ell} (k) \; P _ {\ ell} (\ cos \ vartheta)}
in which
f
ℓ
(
k
)
{\ displaystyle f _ {\ ell} (k)}
the partial scattering amplitude
P
ℓ
(
cos
ϑ
)
{\ displaystyle P _ {\ ell} (\ cos \ vartheta)}
the Legendre polynomial
ℓ
{\ displaystyle \ ell}
is the index for angular momentum.
The partial scattering amplitude can be expressed by the S-matrix element and the scattering phase:
S.
ℓ
=
e
2
i
δ
ℓ
{\ displaystyle S _ {\ ell} = e ^ {2i \ delta _ {\ ell}}}
δ
ℓ
{\ displaystyle \ delta _ {\ ell}}
f
ℓ
=
S.
ℓ
-
1
2
i
k
=
e
2
i
δ
ℓ
-
1
2
i
k
=
e
i
δ
ℓ
sin
δ
ℓ
k
=
1
k
cot
δ
ℓ
-
i
k
.
{\ displaystyle f _ {\ ell} = {\ frac {S _ {\ ell} -1} {2ik}} = {\ frac {e ^ {2i \ delta _ {\ ell}} - 1} {2ik}} = {\ frac {e ^ {i \ delta _ {\ ell}} \ sin \ delta _ {\ ell}} {k}} = {\ frac {1} {k \ cot \ delta _ {\ ell} -ik }} \ ;.}
It should be noted that the partial scattering amplitude , the S-matrix element and the scattering phase are implicit functions of the scattering energy or the momentum .
f
ℓ
{\ displaystyle f _ {\ ell}}
S.
ℓ
=
e
2
i
δ
ℓ
{\ displaystyle S _ {\ ell} = e ^ {2i \ delta _ {\ ell}}}
δ
ℓ
{\ displaystyle \ delta _ {\ ell}}
k
{\ displaystyle k}
The total scattering cross-section can thus be expressed as:
σ
total
=
4th
π
k
2
∑
l
=
0
∞
(
2
l
+
1
)
sin
2
δ
l
.
{\ displaystyle \ sigma _ {\ text {total}} = {\ frac {4 \ pi} {k ^ {2}}} \ sum _ {l = 0} ^ {\ infty} (2l + 1) \ sin ^ {2} \ delta _ {l} \ ;.}
The scatter length can be defined with the help of the partial scatter amplitude:
a
ℓ
{\ displaystyle a _ {\ ell}}
f
ℓ
(
p
)
→
p
→
0
-
a
ℓ
⋅
p
2
ℓ
{\ displaystyle f _ {\ ell} (p) {\ xrightarrow [{p \ rightarrow 0}] {}} - a _ {\ ell} \ cdot p ^ {2 \ ell}}
Usually, however, only the scattering length of the s waves is referred to as the scattering length.
a
0
{\ displaystyle a_ {0}}
(
ℓ
=
0
)
{\ displaystyle (\ ell = 0)}
literature
John R. Taylor: Scattering Theory - The Quantum Theory of Nonrelativistic Collisions, 1983.
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