Stimulated emission of particles by 1+1 dimensional black holes
F. Vendrell (University of Lausanne, Switzerland)

TL;DR
This paper investigates how black holes in 1+1 dimensions stimulate emission of particles, analyzing the thermal and non-thermal radiation properties for different scalar fields and states near the horizon.
Contribution
It provides a comparative study of stimulated emission in relativistic and CGHS black holes, highlighting their thermal and non-thermal radiation characteristics.
Findings
Radiation exhibits both thermal and non-thermal features.
Stimulated emission depends on the initial particle and thermal states.
Differences observed between relativistic and CGHS black hole models.
Abstract
The stimulated emission of massless bosons by a relativistic and the CGHS black hole are studied for real and complex scalar fields. The radiations induced by one-particle and thermal states are considered and their thermal properties investigated near the horizon. These exhibit both thermal and non-thermal properties for the two black-hole models.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Quantum Electrodynamics and Casimir Effect
