Positron bremsstrahlung

I. J. Feng, R. H. Pratt, and H. K. Tseng
Phys. Rev. A 24, 1358 – Published 1 September 1981
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Abstract

Numerical results from a calculation of the positron bremsstrahlung spectrum in a partial-wave expansion are presented for Z=8, 92 at photon energies 10, 50, and 500 keV. Data are presented both for a point-Coulomb potential and for a screened Hartree-Slater central potential. Comparison is made with the corresponding electron bremsstrahlung. In the point-Coulomb case the nonrelativistic Sommerfeld formula or the Elwert factor provides a quantitative prediction of the ratio of the two spectra for Z=8, qualitative for Z=92; similar accuracy is achieved in the screened case with a ratio of screened normalization. The positron spectrum is strongly suppressed for low-energy positrons, which cannot penetrate toward the repulsive central potential. For high-energy positrons or long-distance interactions the positron spectrum approaches the electron spectrum.

  • Received 13 March 1981

DOI:https://doi.org/10.1103/PhysRevA.24.1358

©1981 American Physical Society

Authors & Affiliations

I. J. Feng, R. H. Pratt, and H. K. Tseng*

  • Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15260

  • *Permanent address: Department of Physics, National Central University, Chung-Li, Taiwan, Republic of China.

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Issue

Vol. 24, Iss. 3 — September 1981

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