Abstract
The critical temperature for the 'normal' to 'super-radiant' phase transition and the free energy are modified by the presence of phonons. Results show that whenever there are photons present, there are also phonons.
Radiation damping effects on Dicke's maser model
M Orszag1
Published under licence by IOP Publishing Ltd
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Citation M Orszag 1977 J. Phys. A: Math. Gen. 10 L25
DOI 10.1088/0305-4470/10/1/006
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