UPON THE HORIZON'S VERGE: THERMAL PARTICLE CREATION BETWEEN AND APPROACHING HORIZONS

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dc.contributor.authorFernández-Silvestre, Diego
dc.contributor.authorGood, Michael R R
dc.contributor.authorLinder, Eric V
dc.date.accessioned2023-03-28T10:17:45Z
dc.date.available2023-03-28T10:17:45Z
dc.date.issued2022
dc.description.abstractQuantum particle creation from spacetime horizons, or accelerating boundaries in the dynamical Casimir effect, can have an equilibrium, or thermal, distribution. Using an accelerating boundary in flat spacetime (moving mirror), we investigate the production of thermal energy flux despite non-equilibrium accelerations, the evolution between equilibrium states, and the ‘interference’ between horizons. In particular, this allows us to give a complete solution to the particle spectrum of the accelerated boundary correspondence with Schwarzschild–de Sitter spacetime.en_US
dc.identifier.citationFernández-Silvestre, D., Good, M. R., & Linder, E. V. (2022). Upon the horizon’s verge: Thermal particle creation between and approaching horizons. Classical and Quantum Gravity, 39(23), 235008. https://doi.org/10.1088/1361-6382/ac9d1ben_US
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/6990
dc.language.isoenen_US
dc.publisherClassical and Quantum Gravityen_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 mirrorsen_US
dc.subjectblack hole evaporationen_US
dc.subjectacceleration radiationen_US
dc.subjecthorizonsen_US
dc.titleUPON THE HORIZON'S VERGE: THERMAL PARTICLE CREATION BETWEEN AND APPROACHING HORIZONSen_US
dc.typeArticleen_US
workflow.import.sourcescience

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