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• W3033103511 endingPage "085011" @default.
• W3033103511 startingPage "085011" @default.
• W3033103511 abstract "Abstract An accelerated boundary correspondence (i.e. a flat spacetime accelerating mirror trajectory) is derived for the Kerr spacetime, with a general formula that ranges from the Schwarzschild limit (zero angular momentum) to the extreme maximal spin case (yielding asymptotic uniform acceleration). The beta Bogoliubov coefficients reveal the particle spectrum is a Planck distribution at late times with temperature cooler than a Schwarzschild black hole, due to the ‘spring constant’ analog of angular momentum. The quantum stress tensor indicates a constant emission of energy flux at late times consistent with eternal thermal equilibrium." @default.
• W3033103511 created "2020-06-12" @default.
• W3033103511 creator A5044818705 @default.
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• W3033103511 date "2021-03-18" @default.
• W3033103511 modified "2023-09-27" @default.
• W3033103511 title "Accelerating boundary analog of a Kerr black hole" @default.
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• W3033103511 doi "https://doi.org/10.1088/1361-6382/abebb6" @default.
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