Electron-electron interaction in transition-metal x-ray emission spectra

K. S. Srivastava, Shiv Singh, A. K. Srivastava, R. S. Nayal, Amita Chaubey, and Pratibha Gupta
Phys. Rev. A 25, 2838 – Published 1 May 1982
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Abstract

An alternative explanation for the origin of the Kβ satellite of the Kβ1,3 x-ray emission line of the first transition elements (21Z29) has been given using the Bohm and Pines theory of plasma oscillations in solids. The present calculated values for the energy separation (ΔE), and the relative intensity of the Kβ satellite with respect to the Kβ1,3 x-ray emission line, agree better with the experimentally observed values than the values calculated by the exchange-interaction theory of Tsutsumi et al., Salem et al., and Ekstig et al.

  • Received 23 December 1980

DOI:https://doi.org/10.1103/PhysRevA.25.2838

©1982 American Physical Society

Authors & Affiliations

K. S. Srivastava, Shiv Singh*, A. K. Srivastava, R. S. Nayal, Amita Chaubey, and Pratibha Gupta

  • Theoretical Physics Division, Physics Department, Lucknow University, Lucknow 226007 (U.P.), India

  • *On leave from Physics Department, Hindu College Moradabad 244001, India.

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Vol. 25, Iss. 5 — May 1982

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