MOVING MIRROR MODEL FOR QUASITHERMAL RADIATION FIELDS

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dc.contributor.authorGood, Michael R. R.
dc.contributor.authorLinder, Eric V.
dc.contributor.authorWilczek, Frank
dc.date.accessioned2021-08-26T08:17:07Z
dc.date.available2021-08-26T08:17:07Z
dc.date.issued2020-01-30
dc.description.abstractWe 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.en_US
dc.identifier.citationGood, M. R., Linder, E. V., & Wilczek, F. (2020). Moving mirror model for quasithermal radiation fields. Physical Review D, 101(2). https://doi.org/10.1103/physrevd.101.025012en_US
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/5708
dc.language.isoenen_US
dc.publisherPHYSICAL REVIEW Den_US
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectType of access: Open Accessen_US
dc.subjectMoving mirror modelen_US
dc.titleMOVING MIRROR MODEL FOR QUASITHERMAL RADIATION FIELDSen_US
dc.typeArticleen_US
workflow.import.sourcescience

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