Phys. Rev. Lett. 36, 985–987 (1976)Black Holes in Thermal EquilibriumReceived 1 December 1975; published in the issue dated 19 April 1976 It is argued that a black hole can remain in thermal equilibrium with a heat bath even in the presence of particle interactions. This is achieved by proving the identity of the Hartle-Hawking Feynman propagator and a certain thermal Green's function. © 1976 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevLett.36.985
DOI:
10.1103/PhysRevLett.36.985
PACS:
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