Hawking radiation power equations for black holes

Citation data:

Nuclear Physics B, ISSN: 0550-3213, Vol: 923, Page: 378-393

Publication Year:
2017
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DOI:
10.1016/j.nuclphysb.2017.08.010
Author(s):
Ravi Mistry; Sudhaker Upadhyay; Ahmed Farag Ali; Mir Faizal
Publisher(s):
Elsevier BV
Tags:
Physics and Astronomy
article description
We derive the Hawking radiation power equations for black holes in asymptotically flat, asymptotically Anti-de Sitter (AdS) and asymptotically de Sitter (dS) black holes. This is done by using the greybody factor for these black holes. We observe that the radiation power equation for asymptotically flat black holes, corresponding to greybody factor at low frequency, depends on both the Hawking temperature and the horizon radius. However, for the greybody factors at asymptotic frequency, it only depends on the Hawking temperature. We also obtain the power equation for asymptotically AdS black holes both below and above the critical frequency. The radiation power equation for at asymptotic frequency is same for both Schwarzschild AdS and Reissner–Nordström AdS solutions and only depends on the Hawking temperature. We also discuss the power equation for asymptotically dS black holes at low frequency, for both even or odd dimensions.