Long-Term Solutions in Semiclassical Radiation Theory

C. R. Stroud, Jr. and E. T. Jaynes
Phys. Rev. A 1, 106 – Published 1 January 1970; Erratum Phys. Rev. A 2, 1613 (1970)
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Abstract

An improved form of semiclassical radiation theory is developed which includes the effect of the atom's radiation field back on the atom. This formalism is applied to the problem of a single "two-level atom" interacting with a monochromatic field. The resulting equations are solved without resorting to time-dependent perturbation theory, and are found to predict the behavior of the system over times long compared with the lifetime for spontaneous transitions. Not only stimulated emission and absorption, but also spontaneous emission with the proper Einstein A coefficient, and a frequency shift which agrees at least semiquantitatively with the Lamb shift are described. In addition, several nonlinear effects involving the interference between spontaneous and stimulated radiation are described, and new experiments which might detect such effects are suggested.

  • Received 22 May 1969

DOI:https://doi.org/10.1103/PhysRevA.1.106

©1970 American Physical Society

Erratum

Long-Term Solution in Semiclassical Radiation Theory

C. R. Stroud, Jr. and E. T. Jaynes
Phys. Rev. A 2, 1613 (1970)

Authors & Affiliations

C. R. Stroud, Jr.

  • The Institute of Optics, The University of Rochester, Rochester, New York 14627

E. T. Jaynes

  • Arthur H. Compton Laboratory of Physics, Washington University, St. Louis, Missouri 63130

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Vol. 1, Iss. 1 — January 1970

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