GUP-corrected thermodynamics of accelerating and rotating black holes

Rizwan, Muhammad; Saifullah, Khalid

doi:10.1142/s0218271817410188

Cited by 10 publications

(5 citation statements)

References 39 publications

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“…Using the dragging coordinate transformation, we can avoid the dragging of the spacetime and matter near the event horizon of the black hole [7,37,44,[48][49][50][51][52][53][54][55]. In this context, the metric takes the following form…”

Section: +1 Dimensional Spinning Dilaton Black Holementioning

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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Section: +1 Dimensional Spinning Dilaton Black Holementioning

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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“…Such corrections have been studied for various classes of spacetimes such as for the case of general spherically symmetric metric [19], self dual black holes [20], Reissner-Nordström [21], regular black holes [22], accelerating and rotating black holes [23], and Hořava-Lifshitz gravity [24].…”

Section: Introductionmentioning

confidence: 99%

Thermodynamics of Bardeen regular black hole with generalized uncertainty principle

Merriam,

Sarwar

2021

Preprint

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This study explores the emission of massive charged spin-1 particles from the background of Bardeen regular spacetime by the semi-classical method used to study the Hawking radiation spectrum. We employed the Hamilton-Jacobi method and WKB approximation technique with the suitable form of the wave function to solve the Proca field equation. We calculated the tunneling probability of outgoing spin-1 particles and the corresponding thermodynamic temperature. Furthermore, we obtained the modified thermodynamic quantities like temperature, entropy as well as heat capacity by utilizing the quadratic form of generalized uncertainty principle (GUP) and minimal length. In the end, we investigated the local stability as well as phase transitions of the Bardeen black hole in the context of GUP-modified heat capacity.

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“…In recent years there have been many publications including the effect of GUP [68][69][70][71][72][73][74][75][76][77][78][79][80][81][82][83][84][85][86][87]. Moreover, recently, tunneling of the uncharged particles from rotating black holes has been studied [88], however, there is not completely agreement with the literature.…”

Section: Introductionmentioning

confidence: 99%

Charged fermions tunneling from stationary axially symmetric black holes with generalized uncertainty principle

2019

Self Cite

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In this paper, we study the tunneling of charged fermions from the stationary axially symmetric black holes using the generalized uncertainty principle (GUP) via Wentzel, Kramers, and Brillouin (WKB) method. The emission rate of the charged fermions and corresponding modified Hawking temperature of Ker-Newman black hole, Einstein-Maxwell-Dilaton-Axion (EMDA) black hole, Kaluza-Klein dilaton black hole, and then, charged rotating black string are obtained and we show that the corrected thermal spectrum is not purely thermal because of the minimal scale length which cause the black hole's remnant.

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GUP-corrected thermodynamics of accelerating and rotating black holes

Cited by 10 publications

References 39 publications

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

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

Thermodynamics of Bardeen regular black hole with generalized uncertainty principle

Charged fermions tunneling from stationary axially symmetric black holes with generalized uncertainty principle

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