Charged fermion tunneling from electrically and magnetically charged rotating black hole in de Sitter space

Stetsko, M. M.

doi:10.1140/epjc/s10052-013-2682-5

Cited by 4 publications

(1 citation statement)

References 31 publications

(72 reference statements)

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“…Among them we distinguish Kerr and Kerr-Newman black holes' space-times [8][9][10][11][12], Taub-NUT space-time [13], Gödel space-time [14], BTZ black holes [15,16], dynamical black holes [17], black holes in Hořava-Lifshitz gravity [18,19], accelerating and rotating black holes [20,21], rotating black strings [22], and many others. A review of the tunnelling method is presented in Ref.…”

Section: Introductionmentioning

confidence: 99%

Tunnelling of scalar and Dirac particles from squashed charged rotating Kaluza–Klein black holes

Stetsko

2016

Eur. Phys. J. C

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The thermal radiation of scalar particles and Dirac fermions from squashed charged rotating fivedimensional black holes is considered. To obtain the temperature of the black holes we use the tunnelling method. In the case of scalar particles we make use of the Hamilton-Jacobi equation. To consider tunnelling of fermions the Dirac equation was investigated. The examination shows that the radial parts of the action for scalar particles and fermions in the quasi-classical limit in the vicinity of horizon are almost the same and as a consequence it gives rise to identical expressions for the temperature in the two cases.

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Section: Introductionmentioning

confidence: 99%

Tunnelling of scalar and Dirac particles from squashed charged rotating Kaluza–Klein black holes

Stetsko

2016

Eur. Phys. J. C

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Higher dimensional charged black hole surrounded by quintessence in massive gravity

Nam

2019

Gen Relativ Gravit

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Non-linear charged dS black hole and its thermodynamics and phase transitions

Nam

2018

Eur. Phys. J. C

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From solving the equations of the motion for a system of Einstein gravity coupled to a non-linear electromagnetic field in the dS spacetime with two integral constants, we derived a static and spherical symmetric non-linear magnetic-charged black hole. It is indicated that this black hole solution behaves like a dS geometry in the short-distance regime. And, thus this black hole is regular. The structure of the black hole horizons is studied in detail. Also, we investigated the thermodynamics and the thermal phase transition of the black hole in both the local and global views. By observing the discontinuous change of the specific heat sign and the swallowtail structure of the free energy, we showed that the black hole can undergo a thermal phase transition between a thermodynamically unstable phase and a thermodynamically stable phase.

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Charged fermion tunneling from electrically and magnetically charged rotating black hole in de Sitter space

Cited by 4 publications

References 31 publications

Tunnelling of scalar and Dirac particles from squashed charged rotating Kaluza–Klein black holes

Tunnelling of scalar and Dirac particles from squashed charged rotating Kaluza–Klein black holes

Higher dimensional charged black hole surrounded by quintessence in massive gravity

Non-linear charged dS black hole and its thermodynamics and phase transitions

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