Quantum field theory with and without conical singularities: black holes with a cosmological constant and the multi-horizon scenario
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Publication:4699864
DOI10.1088/0264-9381/16/2/017zbMath0934.83026arXivgr-qc/9708049OpenAlexW2042504938MaRDI QIDQ4699864
Publication date: 18 November 1999
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/9708049
Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20) Methods of quantum field theory in general relativity and gravitational theory (83C47)
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Black hole emission of vector particles in (1+1) dimensions ⋮ Thermodynamics of horizons in a globally regular spherically symmetric spacetime ⋮ Thermodynamics of regular cosmological black holes with the de Sitter interior ⋮ Thermodynamic properties of black holes in de Sitter space ⋮ Some general properties of the renormalized stress-energy tensor for static quantum states on \(( n + 1)\)-dimensional spherically symmetric black holes ⋮ Concept of temperature in multi-horizon spacetimes: analysis of Schwarzschild-de Sitter metric
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