RADIATION FROM AN INERTIAL MIRROR HORIZON

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dc.contributor.authorGood, Michael
dc.contributor.authorAbdikamalov, Ernazar
dc.date.accessioned2021-07-01T13:15:56Z
dc.date.available2021-07-01T13:15:56Z
dc.date.issued2020-08
dc.description.abstractThe purpose of this study is to investigate radiation from asymptotic zero acceleration motion where a horizon is formed and subsequently detected by an outside witness. A perfectly reflecting moving mirror is used to model such a system and compute the energy and spectrum. The trajectory is asymptotically inertial (zero proper acceleration)—ensuring negative energy flux (NEF), yet approaches light-speed with a null ray horizon at a finite advanced time. We compute the spectrum and energy analytically.en_US
dc.identifier.citationGood, M., & Abdikamalov, E. (2020). Radiation from an Inertial Mirror Horizon. Universe, 6(9), 131. doi:10.3390/universe6090131en_US
dc.identifier.issn2218-1997
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/5506
dc.language.isoenen_US
dc.publisherUniverseen_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.subjectacceleration radiationen_US
dc.subjectmoving mirrorsen_US
dc.subjectQFT in curved spacetimeen_US
dc.subjecthorizonsen_US
dc.subjectdynamical Casimir effecten_US
dc.subjectblack holesen_US
dc.subjectHawking radiationen_US
dc.subjectnegative energy fluxen_US
dc.titleRADIATION FROM AN INERTIAL MIRROR HORIZONen_US
dc.typeArticleen_US
workflow.import.sourcescience

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