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Optical hole burning with finite excitation time

From National Research Council Canada

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DOIResolve DOI: https://doi.org/10.1103/PhysRevA.37.4040
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Affiliation
  1. National Research Council of Canada
FormatText, Article
Abstract
This paper extends earlier calculations [M. Yamanoi and J. H. Eberly, Phys. Rev. A 34, 1609 (1986)] of hole burning using continuous excitation to the finite excitation time used in experiments on Pr:LaF3. Both Gaussian-Markov (GM) and random-telegraph (RT) dephasing models are studied. For the GM model, a new feature is the appearance of nutation structure near the center of the hole for a 400-μsec excitation time. In contrast for RT, a similar, although much weaker, structure appears in the wings of the hole. It is noted that for finite excitation times, a detuning as well as the usual intensity dependence of the dephasing time appears.
Publication date
PublisherAmerican Physical Society
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  • Physical Review A 37, no. 10: 4040–4043.
NoteMr. Szabo was affiliated with the National Research Council of Canada, Division of Physics when they authored this article.
LanguageEnglish
Peer reviewedYes
NPARC number23002918
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Record identifier2ceda279-d3da-4bf7-b98c-a74912e2b775
Record created2018-03-23
Record modified2020-05-30
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