Spin One Hawking Radiation from Dirty Black Holes
Commenced in January 2007
Frequency: Monthly
Edition: International
Paper Count: 33122
Spin One Hawking Radiation from Dirty Black Holes

Authors: Petarpa Boonserm, Tritos Ngampitipan, Matt Visser

Abstract:

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.

Keywords: A dirty black hole, Greybody factor, Hawking radiation, Matter fields.

Digital Object Identifier (DOI): doi.org/10.5281/zenodo.1335906

Procedia APA BibTeX Chicago EndNote Harvard JSON MLA RIS XML ISO 690 PDF Downloads 1582

References:


[1] M. Visser, “Dirty black holes: Thermodynamics and horizon structure,” Phys. Rev. D, vol. 46, pp. 2445-2451, September 1992 (hepth/ 9203057).
[2] M. Visser, “Dirty black holes: Entropy versus area,” Phys. Rev. D, vol. 48, pp. 583-591, July 1993 (hep-th/9303029).
[3] M. Visser, “Dirty black holes: Entropy as a surface term,” Phys. Rev. D, vol. 48, pp. 5697-5705, December 1993 (hep-th/9307194).
[4] P. Boonserm and M. Visser, “Bounding the greybody factors for Schwarzschild black holes,” Phys. Rev. D, vol. 78, pp. 101502(R), November 2008 (arXiv:0806.2209 (gr-qc)).
[5] M. Visser, “Some general bounds for one-dimensional scattering,” Phys. Rev. A, vol. 59, pp. 427-438, January 1999 (quant-ph/9901030).
[6] P. Boonserm and M. Visser, “Transmission probabilities and the Miller- Good transformation,” J. Phys. A, vol. 42, pp. 045301, January 2009 (arXiv:0808.2516 (math-ph)).
[7] P. Boonserm and M. Visser, “Analytic bounds on transmission probabilities,” Ann. Phys., vol. 325, pp. 1328-1339, April 2010 (arXiv:0901.0944 (math-ph)).
[8] P. Boonserm and M. Visser, “Reformulating the Schro