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{"references": ["M. Visser, \"Dirty black holes: Thermodynamics and horizon structure,\"\nPhys. Rev. D, vol. 46, pp. 2445-2451, September 1992 (hepth/\n9203057).", "M. Visser, \"Dirty black holes: Entropy versus area,\" Phys. Rev. D, vol.\n48, pp. 583-591, July 1993 (hep-th/9303029).", "M. Visser, \"Dirty black holes: Entropy as a surface term,\" Phys. Rev. D,\nvol. 48, pp. 5697-5705, December 1993 (hep-th/9307194).", "P. Boonserm and M. Visser, \"Bounding the greybody factors for\nSchwarzschild black holes,\" Phys. Rev. D, vol. 78, pp. 101502(R),\nNovember 2008 (arXiv:0806.2209 (gr-qc)).", "M. Visser, \"Some general bounds for one-dimensional scattering,\" Phys.\nRev. A, vol. 59, pp. 427-438, January 1999 (quant-ph/9901030).", "P. Boonserm and M. Visser, \"Transmission probabilities and the Miller-\nGood transformation,\" J. Phys. A, vol. 42, pp. 045301, January 2009\n(arXiv:0808.2516 (math-ph)).", "P. Boonserm and M. Visser, \"Analytic bounds on transmission\nprobabilities,\" Ann. Phys., vol. 325, pp. 1328-1339, April 2010\n(arXiv:0901.0944 (math-ph)).", "P. Boonserm and M. Visser, \"Reformulating the Schro"]}
A “clean” black hole is a black hole in vacuum such as the Schwarzschild black hole. However in real physical systems, there are matter fields around a black hole. Such a black hole is called a “dirty black hole”. In this paper, the effect of matter fields on the black hole and the greybody factor is investigated. The results show that matter fields make a black hole smaller. They can increase the potential energy to a black hole to obstruct Hawking radiation to propagate. This causes the greybody factor of a dirty black hole to be less than that of a clean black hole.
Greybody factor, Hawking radiation, A dirty black hole, Matter fields.
Greybody factor, Hawking radiation, A dirty black hole, Matter fields.
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