Heating up an environment around black holes and inside de Sitter space
arXiv:2010.10877 · doi:10.1103/PhysRevD.103.025023
Abstract
We study quantum fields on spacetimes having a bifurcate Killing horizon by allowing the possibility that left- and right- (in-going and out-going) modes have different temperatures. We consider in particular the Rindler for both massless and massive fields, the static de Sitter and Schwarzschild black hole backgrounds for massive fields. We find that in all three cases, when any of the temperatures is different from the canonical one (Unruh, Hawking and Gibbons--Hawking, correspondingly) the correlation functions have extra singularities at the horizon.
arXiv comment24 pages, 4 figures; The version to appear in PRD, the title has been changed again according to the agreement with the editor
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