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On the line profile coefficient for stimulated emissionIt is pointed out that the line profile coefficients for spontaneous and stimulated emission are identical in low-intensity radiation fields. In more intense radiation fields, however, the stimulated emission profiles in the radiative transfer equation and in the rate equations for the atomic level populations may differ from each other, owing to their different physical nature. A seeming discrepancy between the stimulated emission profiles of the usual semi-classical aproach and a recent quantum mechanical approach by Cooper et al. (1982), which should also be valid for intense 'broadband' fields, is discussed and shown to have negligible consequences for low-intensity radiation fields.
Document ID
19840031353
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Cooper, J.
(Colorado, University; Joint Institute for Laboratory Astrophysics, Boulder, CO, United States)
Hubeny, I.
(Ceskoslovenska Akademie Ved Astronomicky Ustav, Ondrejov, Czechoslovakia)
Oxenius, J.
(Bruxelles, UniversiteLibre Brussels, Belgium)
Date Acquired
August 12, 2013
Publication Date
October 1, 1983
Publication Information
Publication: Astronomy and Astrophysics
Volume: 127
Issue: 1, Oc
ISSN: 0004-6361
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-6361
Accession Number
84A14140
Distribution Limits
Public
Copyright
Other

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