Moving mirror model for quasithermal radiation fields

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 distributi...

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Main Authors: Good, Michael R. R., Linder, Eric V., Wilczek, Frank
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: American Physical Society 2020
Online Access:https://hdl.handle.net/1721.1/125524
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author Good, Michael R. R.
Linder, Eric V.
Wilczek, Frank
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Good, Michael R. R.
Linder, Eric V.
Wilczek, Frank
author_sort Good, Michael R. R.
collection MIT
description 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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spelling mit-1721.1/1255242022-10-02T07:46:05Z Moving mirror model for quasithermal radiation fields Good, Michael R. R. Linder, Eric V. Wilczek, Frank Massachusetts Institute of Technology. Department of Physics 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. European Research Council under Grant No. 742104 Swedish Research Council under Contract No. 335-2014-7424 U.S. Department of Energy under grant Contract No. DE-SC001256 2020-05-27T19:50:37Z 2020-05-27T19:50:37Z 2020-01 2019-10 2020-01-30T16:00:39Z Article http://purl.org/eprint/type/JournalArticle 2470-0029 2470-0010 https://hdl.handle.net/1721.1/125524 Good, Michael R. R., Eric V. Linder, and Frank Wilczek. "Moving mirror model for quasithermal radiation fields." Physical Review D, 101, 2 (January 2020): 025012. © 2020 American Physical Society en http://dx.doi.org/10.1103/PhysRevD.101.025012 Physical Review D Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. American Physical Society application/pdf American Physical Society American Physical Society
spellingShingle Good, Michael R. R.
Linder, Eric V.
Wilczek, Frank
Moving mirror model for quasithermal radiation fields
title Moving mirror model for quasithermal radiation fields
title_full Moving mirror model for quasithermal radiation fields
title_fullStr Moving mirror model for quasithermal radiation fields
title_full_unstemmed Moving mirror model for quasithermal radiation fields
title_short Moving mirror model for quasithermal radiation fields
title_sort moving mirror model for quasithermal radiation fields
url https://hdl.handle.net/1721.1/125524
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