Heating up an environment around black holes and inside de Sitter space

D.V. Diakonov; E.T. Akhmedov; K.V. Bazarov; P.A. Anempodistov; U. Moschella

Heating up an environment around black holes and inside de Sitter space

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arxiv 2010.10877 v3 pith:EECPIBHG submitted 2020-10-21 hep-th

Heating up an environment around black holes and inside de Sitter space

E.T. Akhmedov , P.A. Anempodistov , K.V. Bazarov , D.V. Diakonov , U. Moschella This is my paper

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keywords fieldsblackdifferenthorizonmassivesittertemperaturesallowing

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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.

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Cited by 1 Pith paper

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On the late time behavior of thermal two point function in curved space-time
hep-th 2025-09 conditional novelty 5.0

For thermal Bose fields in static de Sitter or a planar BTZ black hole, the late-time correlation decay switches from temperature-limited to quasinormal-mode-limited at a critical temperature Tc.