MOVING MIRROR MODEL FOR QUASITHERMAL RADIATION FIELDS

dc.contributor.author	Good, Michael R. R.
dc.contributor.author	Linder, Eric V.
dc.contributor.author	Wilczek, Frank
dc.date.accessioned	2021-08-26T08:17:07Z
dc.date.available	2021-08-26T08:17:07Z
dc.date.issued	2020-01-30
dc.identifier.citation	Good, 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.101.025012	en_US
dc.identifier.uri	http://nur.nu.edu.kz/handle/123456789/5708
dc.description.abstract	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.	en_US
dc.language.iso	en	en_US
dc.publisher	PHYSICAL REVIEW D	en_US
dc.rights	Attribution-NonCommercial-ShareAlike 3.0 United States	*
dc.rights.uri	http://creativecommons.org/licenses/by-nc-sa/3.0/us/	*
dc.subject	Type of access: Open Access	en_US
dc.subject	Moving mirror model	en_US
dc.title	MOVING MIRROR MODEL FOR QUASITHERMAL RADIATION FIELDS	en_US
dc.type	Article	en_US
workflow.import.source	science