Upon the horizon's verge: Thermal particle creation between and approaching horizons

Diego Fernández-Silvestre; Michael R. R. Good; Eric V. Linder

doi:10.1088/1361-6382/ac9d1b

Upon the horizon's verge: Thermal particle creation between and approaching horizons

Diego Fernández-Silvestre
, Michael R. R. Good
, Eric V. Linder

School of Sciences and Humanities

Результат исследований › рецензирование

5 Цитирования (Scopus)

8 Загрузки (Pure)

Аннотация

Quantum 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.

Язык оригинала	English
Журнал	Class. Quantum Grav.
DOI	https://doi.org/10.1088/1361-6382/ac9d1b
Состояние	Published - авг. 3 2022

Доступ к документу

10.1088/1361-6382/ac9d1b

2208.01992v2

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AU - Linder, Eric V.

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N2 - Quantum 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.

AB - Quantum 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.

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DO - 10.1088/1361-6382/ac9d1b

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