Vector particles tunneling from four-dimensional Schwarzschild black holes

Chen, Ge-Rui; Zhou, Shiwei; Huang, Yongping

doi:10.1007/s10509-015-2259-x

Cited by 30 publications

(14 citation statements)

References 33 publications

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“…The Hawking temperature corresponding to scalar particle emission is same as the emission temperature of Schwarzschild black hole. Applying Proca equation, many interesting results have been obtained in [25][26][27][28][29][30]. Refs.…”

Section: Introductionmentioning

confidence: 99%

Modified Hawking radiation of stationary and nonstationary Kerr-Newman-de Sitter black hole

Christina,

Singh

2020

Preprint

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In this paper, the tunneling of vector boson particles across the event horizon of Kerr-Newman-de Sitter (KNdS) black hole is investigated using the WKB approximation and Hamilton-Jacobi ansatz to Proca equation. The tunneling probability and radiation spectrum at the event horizon of KNdS black hole is obtained. The modified Hawking radiation of stationary and non-stationary KNdS black hole are also investigated using the Rarita-Schwinger ansatz to the deformed Hamilton-Jacobi method and new tortoise coordinate transformation. It is observed that the modified Hawking temperatures near the event horizon for both stationary and nonstationary space times are dependent on the black hole parameters.

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Section: Introductionmentioning

confidence: 99%

Modified Hawking radiation of stationary and nonstationary Kerr-Newman-de Sitter black hole

Christina,

Singh

2020

Preprint

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“…Nowadays, various methods have been proposed to calculate the temperature of a black hole known as Hawking temperature. On the other hand, the Hamilton-Jacobi approach is an important version of the tunnelling method of the quantum mechanical point-like particles from a black hole [4][5][6][7][8][9][10][11][12][13][14][15][16][17][18][19][20]. Adopting this approach, Hawking temperature of various black holes were recovered by quantum tunnelling method of the particles across their event horizons.…”

Section: Introductionmentioning

confidence: 99%

Quantum gravity effect on the Hawking radiation of spinning dilaton black hole

Geçim

Sucu

2019

Eur. Phys. J. C

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The quantum gravity correction to the Hawking temperature of the 2+1 dimensional spinning dilaton black hole is studied by using the Hamilton-Jacobi approach in the context of the Generalized Uncertainty Principle (GUP). It is observed that the modified Hawking temperature of the black hole depends on both black hole and the tunnelling particle properties. Moreover, it is observed that the mass and the angular momentum of the scalar particle have the same effect on the Hawking temperature of the black hole, while the mass and total angular momentum (orbital+spin) of Dirac particle have different effect. Furthermore, the mass and total angular momentum (orbital+spin) of vector boson particle have a similar effect that of Dirac particle. Also, thermodynamical stability and phase transition of the black hole are discussed for scalar, Dirac and vector boson in the context of GUP, respectively. And, it is observed that the scalar particle probes the black hole as stable whereas, as for Dirac and vector boson particles, it might undergoes secondtype phase transition to become stable while in the absence of the quantum gravity effect all of these particle probes the black hole as stable.

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“…There are various methods for calculating the level of BHR, and the two most popular tunneling methods are the null geodesic method and the Hamilton-Jacobi (HJ) method . Both approaches use the tunneling method by applying the WKB (WentzelKramers-Brillouin) approximation and finding the emission and absorption probabilities of the tunneling particles, which give the tunneling rate Γ as follows [40][41][42][43][44][45][46][47][48][49][50][51]:…”

Section: Introductionmentioning

confidence: 99%

The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole

Овгун

2017

Advances in High Energy Physics

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Exciting peculiarities of Planck-scale physics have immediate effects on the Bekenstein-Hawking radiation emitted from black holes (BHs). In this paper, using the tunneling formalism, we determine the Bekenstein-Hawking temperature for the vector particles from a back-reacted black hole (BBH) constructed from a conformal scalar field surrounded by a BTZ (Banados-Teitelboim-Zanelli) BH. Then, under the effect of the generalized uncertainty principle, we extend our calculations for scalar particles to understand the effects of quantum gravity. Then, we calculate an evaporation time for the BBH, the total number of Bekenstein-Hawking particles, and the quantum corrections of the number. We observe that remnants of the BH evaporation occur and that they affect the Bekenstein-Hawking temperature of the BBH as well as the total number of Bekenstein-Hawking particles.

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Vector particles tunneling from four-dimensional Schwarzschild black holes

Cited by 30 publications

References 33 publications

Modified Hawking radiation of stationary and nonstationary Kerr-Newman-de Sitter black hole

Modified Hawking radiation of stationary and nonstationary Kerr-Newman-de Sitter black hole

Quantum gravity effect on the Hawking radiation of spinning dilaton black hole

The Bekenstein-Hawking Corpuscular Cascading from the Back-Reacted Black Hole

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