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Scattering amplitude : ウィキペディア英語版
Scattering amplitude

In quantum physics, the scattering amplitude is the amplitude of the outgoing spherical wave relative to the incoming plane wave in a stationary-state scattering process.〔(Quantum Mechanics: Concepts and Applications By Nouredine Zettili, 2nd edition, page 623. ISBN 978-0-470-02679-3 Paperback 688 pages January 2009, ©2008 )〕 The latter is described by the wavefunction
:
\psi(\mathbf) = e^ + f(\theta)\frac \;,

where \mathbf\equiv(x,y,z) is the position vector; r\equiv|\mathbf|; e^ is the incoming plane wave with the wavenumber k along the z axis; e^/r is the outgoing spherical wave; \theta is the scattering angle; and f(\theta) is the scattering amplitude. The dimension of the scattering amplitude is length.
The scattering amplitude is a probability amplitude and the differential cross-section as a function of scattering angle is given as its modulus squared
:
\frac = |f(\theta)|^2 \;.

In the low-energy regime the scattering amplitude is determined by the scattering length.
== Partial wave expansion ==

(詳細はMichael Fowler/ 1/17/08 Plane Waves and Partial Waves )〕
:f=\sum_^\infty (2\ell+1) f_\ell P_\ell(\cos \theta),
where is the partial scattering amplitude and are the Legendre polynomials.
The partial amplitude can be expressed via the partial wave S-matrix element (=e^) and the scattering phase shift as
:f_\ell = \frac = \frac = \frac = \frac \;.
Then the differential cross section is given by
:\frac = |f(\theta)|^2 = \frac \left| \sum_^\infty (2\ell+1) e^ \sin \delta_\ell P_\ell(\cos \theta) \right|^2,
and the total elastic cross section becomes
:\sigma = 2 \pi \int_0^\pi \frac \sin \theta \, d \theta = \frac \operatorname f(0),
where is the imaginary part of .

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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