Moving mirror model for quasithermal radiation fields

Good, Michael R. R.; Linder, Eric V.; Wilczek, Frank

doi:10.1103/PhysRevD.101.025012

Moving mirror model for quasithermal radiation fields

Journal Article · Thu Jan 30 00:00:00 EST 2020 · Physical Review D

DOI:https://doi.org/10.1103/PhysRevD.101.025012· OSTI ID:1635008

Good, Michael R. R. ^[1]; ^[2]; Wilczek, Frank ^[3]

Nazarbayev Univ., Astana (Kazakhstan); Massachusetts Institute of Technology (MIT), Cambridge, MA (United States)
Nazarbayev Univ., Astana (Kazakhstan); Univ. of California, Berkeley, CA (United States)
Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States); Shanghai Jiao Tong Univ. (China); Arizona State Univ., Tempe, AZ (United States); Stockholm Univ. (Sweden)

We analyze the flow of energy and entropy emitted by a class of moving mirror trajectories which provide models for important aspects of the radiation fields produced by black hole evaporation. The mirror radiation fields provide natural, concrete examples of processes that follow thermal distributions for long periods, accompanied by transients which are brief and carry little net energy, yet ultimately represent pure quantum states. In conclusion, a burst of negative energy flux is a generic feature of these fields, but it need not be prominent.

View Accepted Manuscript (DOE)

Research Organization:: Massachusetts Institute of Technology (MIT), Cambridge, MA (United States)

Sponsoring Organization:: Swedish Research Council; USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)

Grant/Contract Number:: AC02-05CH11231; SC0007867; SC0012567

OSTI ID:: 1635008

Journal Information:: Physical Review D, Journal Name: Physical Review D Journal Issue: 2 Vol. 101; ISSN PRVDAQ; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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