Accurate calculation of dynamic Stark shifts and depopulation rates of Rydberg energy levels induced by blackbody radiation. Hydrogen, helium, and alkali-metal atoms

John W. Farley and William H. Wing
Phys. Rev. A 23, 2397 – Published 1 May 1981
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Abstract

A highly excited (Rydberg) atom bathed in blackbody radiation is perturbed in two ways. A dynamic Stark shift is induced by the off-resonant components of the blackbody radiation. Additionally, electric-dipole transitions to other atomic energy levels are induced by the resonant components of the blackbody radiation. This depopulation effect shortens the Rydberg-state lifetime, thereby broadening the energy level. Calculations of these two effects in many states of hydrogen, helium, and the alkali-metal atoms Li, Na, K, Rb, and Cs are presented for T=300 K. Contributions from the entire blackbody spectrum and from both discrete and continuous perturbing states are included. The accuracy is considerably greater than that of previous estimates.

  • Received 6 June 1980

DOI:https://doi.org/10.1103/PhysRevA.23.2397

©1981 American Physical Society

Authors & Affiliations

John W. Farley

  • Department of Physics and Optical Sciences Center, University of Arizona, Tucson, Arizona 85721

William H. Wing

  • Joint Institute for Laboratory Astrophysics, Boulder, Colorado 80309 and Department of Physics and Optical Sciences Center, University of Arizona, Tucson, Arizona 85721

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Vol. 23, Iss. 5 — May 1981

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