Physics:Scattering amplitude

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Short description: Probability amplitude in quantum scattering theory

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 k along the z axis; eikr/r is the outgoing spherical wave; θ 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 form[2]

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 have[2]

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).[2]

Partial wave expansion

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 f is the partial scattering amplitude and P are the Legendre polynomials. The partial amplitude can be expressed via the partial wave S-matrix element S (=e2iδ) and the scattering phase shift δ as

f=S12ik=e2iδ12ik=eiδsinδk=1kcotδik.

Then the total cross section[4]

σ=|f(θ)|2dΩ,

can be expanded as[2]

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 write[2]

f=12ik=0(2+1)e2iδlP(cosθ).

X-rays

The scattering length for X-rays is the Thomson scattering length or classical electron radius, r0.

Neutrons

The nuclear neutron scattering process involves the coherent neutron scattering length, often described by b.

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

  1. Quantum Mechanics: Concepts and Applications By Nouredine Zettili, 2nd edition, page 623. ISBN:978-0-470-02679-3 Paperback 688 pages January 2009
  2. 2.0 2.1 2.2 2.3 2.4 2.5 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. Schiff, Leonard I. (1968). Quantum Mechanics. New York: McGraw Hill. pp. 119–120. https://archive.org/details/quantummechanics00schi_086.