Vector particles tunneling from BTZ black holes

Chen, Ge-Rui; Zhou, Shiwei; Huang, Yong-Chang

doi:10.1142/s0218271815500054

Cited by 29 publications

(20 citation statements)

References 13 publications

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“…which is also equivalent to the Boltzmann factor: exp(−E net /T ) [8,11,26]. From this point on, we can compute the surface temperature of the event horizon of WAdS 3 BH as .…”

Section: Quantum Tunneling Of Vector Particles From Wads3bhsmentioning

confidence: 99%

Hawking radiation of massive vector particles from a warped AdS₃ black hole

Gürsel

Сакалли

2016

Can. J. Phys.

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Hawking radiation (HR) of massive vector particles from a rotating Warped Anti-de Sitter black hole in 2+1 dimensions (WAdS3BH) is studied in detail. The quantum tunneling approach with the Hamilton-Jacobi method (HJM) is applied in the Proca equation (PE), and we show that the radial function yields the tunneling rate of the outgoing particles. Comparing the result obtained with the Boltzmann factor, we satisfactorily reproduce the Hawking temperature (HT) of the WAdS3BH.

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“…which is also equivalent to the Boltzmann factor: exp(−E net /T ) [8,11,26]. From this point on, we can compute the surface temperature of the event horizon of WAdS 3 BH as .…”

Section: Quantum Tunneling Of Vector Particles From Wads3bhsmentioning

confidence: 99%

Hawking radiation of massive vector particles from a warped AdS₃ black hole

Gürsel

Сакалли

2016

Can. J. Phys.

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“…Moreover, the Hawking temperature of BH increases due to the rotation parameter. Furthermore, our analysis is similar to the analysis for charged scalar and fermion particles tunneling from these BHs [59][60][61][62][63]. The charged scalar and fermion particles radiate through the BHs horizons with the same energy.…”

Section: Discussionmentioning

confidence: 58%

Tunneling of Massive Vector Particles from Types of BTZ-like Black Holes

Javed¹,

Ali²,

Babar³

et al. 2019

Preprint

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In this paper, we analyze the Hawking radiation phenomenon for types of Banados-Teitelboim-Zanelli-like (BTZ-like) black holes. For this purpose, using the Hamilton-Jacobi method, we consider semi-classical WKB approximation to calculate the tunneling probabilities of massive boson particles. For these particles, we use the equation of motion for the Glashow-Weinberg-Salam model. Using quantum tunneling process of charged massive bossons, we compute the corresponding Hawking temperatures. Furthermore, we discuss the effects of rotation parameter on tunneling probability and temperature.

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“…From these methods, the Hamilton-Jacobi method, based on quantum tunneling process of a particle, is the most popular method [17][18][19][20][21][22][23][24][25][26][27]. By using the Hamilton-Jacobi approach, Hawking radiations of a number of black holes as quantum tunneling process of a point particle have been investigated in the literature [28][29][30][31][32][33][34][35][36][37][38][39][40]. Recently, it has been also showed that Elko (dark) particles which are spin-1/2 fermions of mass dimension one and dual-helicity eigen spinors of the charge conjugation operator are emitted at the expected Hawking temperature from black holes and strings [39,40].…”

Section: Introductionmentioning

confidence: 99%

Quantum Gravity Correction to Hawking Radiation of the 2+1-Dimensional Wormhole

Geçim

Sucu

2020

Advances in High Energy Physics

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We carry out the Hawking temperature of a 2+1-dimensional circularly symmetric traversable wormhole in the framework of the generalized uncertainty principle (GUP). Firstly, we introduce the modified Klein-Gordon equation of the spin-0 particle, the modified Dirac equation of the spin-1/2 particle, and the modified vector boson equation of the spin-1 particle in the wormhole background, respectively. Given these equations under the Hamilton-Jacobi approach, we analyze the GUP effect on the tunneling probability of these particles near the trapping horizon and, subsequently, on the Hawking temperature of the wormhole. Furthermore, we have found that the modified Hawking temperature of the wormhole is determined by both wormhole’s and tunneling particle’s properties and indicated that the wormhole has a positive temperature similar to that of a physical system. This case indicates that the wormhole may be supported by ordinary (nonexotic) matter. In addition, we calculate the Unruh-Verlinde temperature of the wormhole by using Kodama vectors instead of time-like Killing vectors and observe that it equals to the standard Hawking temperature of the wormhole.

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Vector particles tunneling from BTZ black holes

Abstract: In this paper we investigate vector particles' Hawking radiation from a BTZ black hole. By applying the WKB approximation and the Hamilton-Jacobi Ansatz to the Proca equation, we obtain the tunneling spectrum of vector particles. The expected Hawking temperature is recovered

Cited by 29 publications

References 13 publications

Hawking radiation of massive vector particles from a warped AdS₃ black hole

Hawking radiation of massive vector particles from a warped AdS₃ black hole

Tunneling of Massive Vector Particles from Types of BTZ-like Black Holes

Quantum Gravity Correction to Hawking Radiation of the 2+1-Dimensional Wormhole

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Vector particles tunneling from BTZ black holes

Abstract: In this paper we investigate vector particles' Hawking radiation from a BTZ black hole. By applying the WKB approximation and the Hamilton-Jacobi Ansatz to the Proca equation, we obtain the tunneling spectrum of vector particles. The expected Hawking temperature is recovered

Cited by 29 publications

References 13 publications

Hawking radiation of massive vector particles from a warped AdS3 black hole

Hawking radiation of massive vector particles from a warped AdS3 black hole

Tunneling of Massive Vector Particles from Types of BTZ-like Black Holes

Quantum Gravity Correction to Hawking Radiation of the 2+1-Dimensional Wormhole

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Product

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Hawking radiation of massive vector particles from a warped AdS₃ black hole

Hawking radiation of massive vector particles from a warped AdS₃ black hole