Journal
PHYSICAL REVIEW D
Volume 101, Issue 2, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.101.025012
Keywords
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Funding
- ORAU FY2018-SGP-1-STMM Faculty Development Competitive Research Grant at Nazarbayev University [090118FD5350]
- state-targeted program Center of Excellence for Fundamental and Applied Physics by the Ministry of Education and Science of the Republic of Kazakhstan [BR05236454]
- Energetic Cosmos Laboratory
- U.S. Department of Energy, Office of Science, Office of High Energy Physics [DE-SC-0007867, DE-AC02-05CH11231]
- U.S. Department of Energy [DE-SC0012567]
- European Research Council [742104]
- Swedish Research Council [335-2014-7424]
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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. A burst of negative energy flux is a generic feature of these fields, but it need not be prominent.
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