Scattering amplitude

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Template:Use American English Template:Short description In quantum physics, the scattering amplitude is the probability amplitude of the outgoing spherical wave relative to the incoming plane wave in a stationary-state scattering process.[1] At large distances from the centrally symmetric scattering center, the plane wave is described by the wavefunction[2]

ψ(𝐫)=eikz+f(θ)eikrr,

where 𝐫(x,y,z) is the position vector; r|𝐫|; eikz is the incoming plane wave with the wavenumber Template:Mvar along the Template:Mvar axis; eikr/r is the outgoing spherical wave; Template:Mvar is the scattering angle (angle between the incident and scattered direction); and f(θ) is the scattering amplitude. The dimension of the scattering amplitude is length. The scattering amplitude is a probability amplitude; the differential cross-section as a function of scattering angle is given as its modulus squared,

dσ=|f(θ)|2dΩ.

The asymptotic form of the wave function in arbitrary external field takes the formTemplate:R

ψ=eikr𝐧𝐧+f(𝐧,𝐧)eikrr

where 𝐧 is the direction of incidient particles and 𝐧 is the direction of scattered particles.

Unitary condition

When conservation of number of particles holds true during scattering, it leads to a unitary condition for the scattering amplitude. In the general case, we haveTemplate:R

f(𝐧,𝐧)f*(𝐧,𝐧)=ik2πf(𝐧,𝐧)f*(𝐧,𝐧)dΩ

Optical theorem follows from here by setting 𝐧=𝐧.

In the centrally symmetric field, the unitary condition becomes

Imf(θ)=k4πf(γ)f(γ)dΩ

where γ and γ are the angles between 𝐧 and 𝐧 and some direction 𝐧. This condition puts a constraint on the allowed form for f(θ), i.e., the real and imaginary part of the scattering amplitude are not independent in this case. For example, if |f(θ)| in f=|f|e2iα is known (say, from the measurement of the cross section), then α(θ) can be determined such that f(θ) is uniquely determined within the alternative f(θ)f*(θ).Template:R

Partial wave expansion

Template:Main article

In the partial wave expansion the scattering amplitude is represented as a sum over the partial waves,[3]

f==0(2+1)fP(cosθ),

where Template:Math is the partial scattering amplitude and Template:Math are the Legendre polynomials. The partial amplitude can be expressed via the partial wave S-matrix element Template:Math (=e2iδ) and the scattering phase shift Template:Math as

f=S12ik=e2iδ12ik=eiδsinδk=1kcotδik.

Then the total cross section[4]

σ=|f(θ)|2dΩ,

can be expanded asTemplate:R

σ=l=0σl,whereσl=4π(2l+1)|fl|2=4πk2(2l+1)sin2δl

is the partial cross section. The total cross section is also equal to σ=(4π/k)Imf(0) due to optical theorem.

For θ0, we can writeTemplate:R

f=12ik=0(2+1)e2iδlP(cosθ).

X-rays

The scattering length for X-rays is the Thomson scattering length or classical electron radius, Template:Mvar0.

Neutrons

The nuclear neutron scattering process involves the coherent neutron scattering length, often described by Template:Mvar.

Quantum mechanical formalism

A quantum mechanical approach is given by the S matrix formalism.

Measurement

The scattering amplitude can be determined by the scattering length in the low-energy regime.

See also

References

Template:Reflist

  1. ↑ Quantum Mechanics: Concepts and Applications Template:Webarchive By Nouredine Zettili, 2nd edition, page 623. Template:ISBN Paperback 688 pages January 2009
  2. ↑ Landau, L. D., & Lifshitz, E. M. (2013). Quantum mechanics: non-relativistic theory (Vol. 3). Elsevier.
  3. ↑ Michael Fowler/ 1/17/08 Plane Waves and Partial Waves
  4. ↑ Template:Cite book