Black Holes and Thermal Green Functions Export

@article{citeulike:6032120, abstract = {This paper concerns itself with the possibility of thermal equilibrium between a black hole and a heat bath implied by Hawking's discovery of black hole emission. We argue that in an isolated box of radiation, for sufficiently high energy density a black hole will condense out. We introduce thermal Green functions to discuss this equilibrium and are able to extend the original arguments, that the equilibrium is possible based on fields interacting solely with the external gravitational field, to the case when mutual and self interactions are included.}, author = {Gibbons, G. W. and Perry, M. J.}, citeulike-article-id = {6032120}, citeulike-linkout-0 = {http://dx.doi.org/10.2307/79482}, citeulike-linkout-1 = {http://www.jstor.org/stable/79482}, doi = {10.2307/79482}, issn = {00804630}, journal = {Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences}, keywords = {gr, green-function, hawking-effect, hawking-hartle-vacuum, qft, schwarzschild, thermal}, number = {1695}, pages = {467--494}, posted-at = {2009-10-29 13:32:39}, priority = {0}, publisher = {The Royal Society}, title = {Black Holes and Thermal Green Functions}, url = {http://dx.doi.org/10.2307/79482}, volume = {358}, year = {1978} }

TY - JOUR ID - citeulike:6032120 L3 - citeulike-article-id:6032120 N2 - This paper concerns itself with the possibility of thermal equilibrium between a black hole and a heat bath implied by Hawking's discovery of black hole emission. We argue that in an isolated box of radiation, for sufficiently high energy density a black hole will condense out. We introduce thermal Green functions to discuss this equilibrium and are able to extend the original arguments, that the equilibrium is possible based on fields interacting solely with the external gravitational field, to the case when mutual and self interactions are included. IS - 1695 JF - Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences SN - 00804630 EP - 494 TI - Black Holes and Thermal Green Functions PB - The Royal Society VL - 358 SP - 467 KW - gr KW - green-function KW - hawking-effect KW - hawking-hartle-vacuum KW - qft KW - schwarzschild KW - thermal AU - Gibbons, GW AU - Perry, MJ PY - 1978/// UR - http://dx.doi.org/10.2307/79482 ER -