Quantum optics meets black hole thermodynamics via conformal quantum
mechanics: I. Master equation for acceleration radiation
- URL: http://arxiv.org/abs/2108.07570v1
- Date: Tue, 17 Aug 2021 11:44:30 GMT
- Title: Quantum optics meets black hole thermodynamics via conformal quantum
mechanics: I. Master equation for acceleration radiation
- Authors: A. Azizi, H. E. Camblong, A. Chakraborty, C. R. Ordonez, and M. O.
Scully
- Abstract summary: A quantum-optics approach is used to study the nature of the acceleration radiation due to a random atomic cloud falling into a generalized Schwarzschild black hole.
The properties of this horizon brightened acceleration radiation (HBAR) are analyzed with a master equation that is fully developed in a multimode format.
- Score: 0.0
- License: http://creativecommons.org/licenses/by/4.0/
- Abstract: A quantum-optics approach is used to study the nature of the acceleration
radiation due to a random atomic cloud falling freely into a generalized
Schwarzschild black hole through a Boulware vacuum. The properties of this
horizon brightened acceleration radiation (HBAR) are analyzed with a master
equation that is fully developed in a multimode format. A scheme for the
coarse-graining average for an atomic cloud is considered, with emphasis on the
random injection scenario, which is shown to generate a thermal state. The role
played by conformal quantum mechanics (CQM) is shown to be critical for
detailed balance via a Boltzmann factor governed by the near-horizon physics,
with the unique selection of the Hawking temperature. The HBAR thermal state is
the basis for a thermodynamic framework that parallels black hole
thermodynamics.
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