Hawking radiation of charged particles as tunneling from Reissner–Nordström–de Sitter black holes with a global monopole
152 citations recorded by the source corpus.
Abstract Applying Parikh's semi-classical tunneling method, we consider Hawking radiation of the charged massive particles as a tunneling process from the Reissner–Nordstrom–de Sitter black hole with a global monopole. The result shows that the tunneling rate is related to the change of Bekenstein–Hawking entropy and the radiant spectrum is not a pure thermal one, but is consistent with an underlying unitary theory.
View Paper: https://www.semanticscholar.org/paper/a7b8c3f9040a702d85b923e36fb3bcf77e9275dc
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- Bibhas Ranjan Majhi
- R. Banerjee
- Saurav Samanta
- Ashoke Sen
- Kourosh Nozari
- Sujoy K. Modak
Citations in the corpus
- Remarks on Hawking radiation as tunneling from the BTZ black holes (2006, unknown): “Ever since Parikh and Wilczek [1] put forward a semiclassica l framework (see also [2] for early works underlying the basis of this framework) to imple ment Hawking radiation as a tunneling process across the horizon of the static spherically symmet ric black holes and demonstrated that the emission”
- Quantum tunneling beyond semiclassical approximation (2008, background): “There are some papers [32, 33] in which this case is analysed.”
- Noncommutative black hole thermodynamics (2008, methodology): “In this paper we derive the relation Th = K 2π using the tunneling approach, thereby making redundant independent calculations of the Hawking temperature for different metrics [5].”