A simplified derivation of stimulated emission by black holes

Details A simplified derivation of stimulated emission by black holes A simplified derivation of stimulated emission by black holes

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cqgra...4l.149s&link_type=abstract

Classical and Quantum Gravity (ISSN 0264-9381), vol. 4, July 1, 1987, p. L149-L155. NASA-supported research.

Astronomy and Astrophysics

Astronomy

2

Black Holes (Astronomy), Gibbs Free Energy, Radiation Distribution, Stimulated Emission

Scientific paper

A black hole, when acting as a scatterer for quanta in a single mode of a massless scalar field, is known to convert any ingoing Gibbs state of that mode into an outgoing Gibbs state (with some other mean particle number). The paper presents a simple derivation for this property which may help to clarify what relation, if any, it bears to the microscopic structure of the black hole horizon.

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