The Quantum Tunneling Effect of Internal Global Monopole Black Hole

2012 ◽  
Vol 170-173 ◽  
pp. 2991-2994
Author(s):  
Qing Quan Jiang
Keyword(s):  
Black Hole ◽  
Energy Conservation ◽  
Event Horizon ◽  
Quantum Tunneling ◽  
Tunneling Effect ◽  
Global Monopole

Considering energy conservation, the tunneling effect of internal global monopole black hole is deeply studied in the Parikh-Wilczek’s tunneling framework. The result shows that the emission of the particle on the event horizon is relation to the change of Bekenstein-Hawking entropy and the spectrum is a not pure thermal one.

DISCUSSION ON THE CHARACTERISTICS OF THE QUANTUM TUNNELING RADIATION OF GLOBAL MONOPOLE CHARGED BLACK HOLE

2006 ◽  
Vol 21 (07) ◽  
pp. 1529-1535 ◽  
Author(s):  
DE-JIANG QI ◽  
HUI-LING LI ◽  
QING-QUAN JIANG ◽  
MEN-QUAN LIU ◽  
SHU-ZHENG YANG
Keyword(s):  
Black Hole ◽  
Energy Conservation ◽  
Event Horizon ◽  
Quantum Tunneling ◽  
Charged Black Hole ◽  
Tunneling Effect ◽  
Global Monopole ◽  
Tunneling Radiation

Considering energy conservation, adopting KKW method, the tunneling effect of global monopole charged black hole was deeply studied. The result shows that the emission of particle on the event horizon relates to the change of Bekenstein–Hawking entropy and the spectrum is not pure thermal. Moreover, the corrections to the entropy and temperature of the black hole are presented.

scholarly journals The Accurate Modification of Tunneling Radiation of Fermions with Arbitrary Spin in Kerr-de Sitter Black Hole Space-Time

2020 ◽  
Vol 2020 ◽  
pp. 1-6 ◽  
Author(s):  
Bei Sha ◽  
Zhi-E Liu ◽  
Xia Tan ◽  
Yu-Zhen Liu ◽  
Jie Zhang
Keyword(s):  
Black Hole ◽  
Dispersion Relation ◽  
String Theory ◽  
Event Horizon ◽  
Quantum Tunneling ◽  
Gravitational Theory ◽  
Arbitrary Spin ◽  
Space Time ◽  
De Sitter ◽  
Tunneling Radiation

The quantum tunneling radiation of fermions with arbitrary spin at the event horizon of Kerr-de Sitter black hole is accurately modified by using the dispersion relation proposed in the study of string theory and quantum gravitational theory. The derived tunneling rate and temperature at the black hole horizons are analyzed and studied.

scholarly journals Quantum tunneling approach of noncommutative geometry

2019 ◽  
Author(s):  
Vitaly Kuyukov
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Quantum Information ◽  
Minkowski Space ◽  
Event Horizon ◽  
Noncommutative Geometry ◽  
Quantum Tunneling ◽  
Holographic Principle ◽  
Minkowski Space Time ◽  
Thermodynamics Of Black Holes

Hawking and Beckenstein’s theory of the thermodynamics of black holes indicates that there is a connection between quantum information and gravity. In general, their result is called the holographic principle. According to it, the entropy of a black hole is proportional to the area of the sphere of the event horizon. In this paper, noncommutative geometry is generalized using the holographic principle. Under certain assumptions, it is possible to obtain results from this synthesis regarding the geometry of the Minkowski space-time. To do this, we consider two main provisions for the generalization of noncommutative geometry.

Fermion tunneling, Instability and First Law of Rindler Modified Schwarzschild Black Hole as a Thermodynamic system

2020 ◽  
Author(s):  
S. Fatemeh Mirekhtiary ◽  
I. Sakalli ◽  
V. Bashiry
Keyword(s):  
Thermal Stability ◽  
Black Hole ◽  
Cosmological Constant ◽  
Event Horizon ◽  
Quantum Tunneling ◽  
Thermodynamic System ◽  
Unstable System ◽  
Schwarzschild Black Hole ◽  
Rindler Acceleration ◽  
Thermal Stability Of

This study investigated quantum tunneling of spin half particles through the event horizon of Rindler modified Schwarzschild black hole (RMSBH) in the presence of quintessence matter. We analyzed the thermodynamics of RMSBH in the Kiselev coordinates. Particularly, exploring RMSBH's entropy and the thermal stability of the RMSBH. We showed that RMSBH serves an unstable system causing fluctuations. The integral formulation of the first law of RMSBH in the absence of cosmological constant was also represented. By using the first law, we finally studied the Ruppeiner geometry for Rindler acceleration and pressure with fixed ensembles .

scholarly journals The quantum tunneling effect of Reissner-Nordstr?m de Sitter black hole

2006 ◽  
Vol 55 (2) ◽  
pp. 539
Author(s):  
Li Hui-Ling ◽  
Jiang Qing-Quan ◽  
Yang Shu-Zheng
Keyword(s):  
Black Hole ◽  
Quantum Tunneling ◽  
Tunneling Effect ◽  
De Sitter

scholarly journals Quantum tunneling approach of noncommutative geometry

2019 ◽  
Author(s):  
Vitaly Kuyukov
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Quantum Information ◽  
Minkowski Space ◽  
Event Horizon ◽  
Noncommutative Geometry ◽  
Quantum Tunneling ◽  
Holographic Principle ◽  
Minkowski Space Time ◽  
Thermodynamics Of Black Holes

Hawking and Beckenstein’s theory of the thermodynamics of black holes indicates that there is a connection between quantum information and gravity. In general, their result is called the holographic principle. According to it, the entropy of a black hole is proportional to the area of the sphere of the event horizon. In this paper, noncommutative geometry is generalized using the holographic principle. Under certain assumptions, it is possible to obtain results from this synthesis regarding the geometry of the Minkowski space-time. To do this, we consider two main provisions for the generalization of noncommutative geometry.

scholarly journals Black hole emission of vector particles in (1+1) dimensions

2014 ◽  
Vol 29 (22) ◽  
pp. 1450118 ◽  
Author(s):  
S. I. Kruglov
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Event Horizon ◽  
Quantum Tunneling ◽  
De Sitter Space ◽  
Space Time ◽  
De Sitter ◽  
Proca Equation ◽  
Scalar Particles ◽  
Vector Particles

We investigate the radiation of spin-1 particles by black holes in (1+1) dimensions within the Proca equation. The process is considered as quantum tunneling of bosons through an event horizon. It is shown that the emission temperature for the Schwarzschild background geometry is the same as the Hawking temperature corresponding to scalar particles emission. We also obtain the radiation temperatures for the de Sitter, Rindler and Schwarzschild–de Sitter space–times. In a particular case when two horizons in Schwarzschild–de Sitter space–time coincides, the Nariai temperature is recovered. The thermodynamical entropy of a black hole is calculated for Schwarzschild–de Sitter space–time having two horizons.

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