Elastic scattering of photons by K-shell electrons at high energies

V. Florescu and M. Gavrila
Phys. Rev. A 14, 211 – Published 1 July 1976
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Abstract

The matrix element for Rayleigh scattering by atomic K-shell electrons is evaluated in the limit of high photon energies at finite momentum transfers Δ. The limiting form of the matrix element M¯ is derived from its relativistic expression at finite energies M in which the one-electron Green's function G is replaced by its nonrelativistic approximation G0 with adequately modified parameters. The expression obtained for M¯ is exact in Δ and the atomic number Z, and is equivalent to the one found by Goldberger and Low. The evaluation of the matrix element is carried out in momentum space for the case of a Coulomb atomic field. Exact integral representations are used for G0 and the ground-state eigenspinors. The integration of M is carried out analytically as far as possible and at one stage the high-energy limit is taken. For one K-shell electron, when electron spin-flip is possible, M¯ is expressed in terms of three real amplitudes H, K, and L, whereas the matrix element for the closed K shell, M¯K, depends only on H. The amplitudes are obtained as one-dimensional integrals over Appell functions F1. They simplify considerably in the case of forward scattering, and the connection of their imaginary parts with absorption cross sections is discussed. Expansions of the forward amplitudes in powers of a=αZ are also given. Further, a connection between H and the nonrelativistic form factor is established, and the asymptotic behavior of H with respect to Δ is derived. Then, a description is given of the numerical methods used. H is computed for 0Δam15 and 1Zα1. Of the electron spin-flip amplitudes only K is computed for forward scattering (L vanishes in this case). The numerical results are discussed and comparison is made with other works. The validity of the high-energy result M¯K at lower photon energies is considered. Finally, the magnitude of the Rayleigh matrix element M¯K is compared with the one for Delbrück scattering.

  • Received 29 December 1975

DOI:https://doi.org/10.1103/PhysRevA.14.211

©1976 American Physical Society

Authors & Affiliations

V. Florescu and M. Gavrila

  • Department of Physics, University of Pittsburgh, Pittsburgh, Pennsylvania 15260
  • Department of Physics, University of Bucharest, Bucharest, Romania

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Issue

Vol. 14, Iss. 1 — July 1976

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