scholarly journals A new method for exploring the black hole Hawking radiation——the quantum statistical method

2006 ◽  
Vol 55 (8) ◽  
pp. 3898
Author(s):  
Zhao Ren ◽  
Zhang Li-Chun ◽  
Hu Shuang-Qi
2018 ◽  
Vol 33 (32) ◽  
pp. 1850185 ◽  
Author(s):  
M. A. Anacleto ◽  
Ines G. Salako ◽  
F. A. Brito ◽  
E. Passos

In this paper, we consider the metric of a (2[Formula: see text]+[Formula: see text]1)-dimensional rotating acoustic black hole in the neo-Newtonian theory to compute the Hawking temperature, and applying the quantum statistical method, we calculate the statistical entropy using a corrected state density due to the generalized uncertainty principle (GUP). In our calculations, we have shown that the obtained entropy is finite and correction terms are generated. Moreover, the computation of the entropy for this method does not present logarithmic corrections.


2012 ◽  
Vol 51 (12) ◽  
pp. 3805-3814
Author(s):  
M. Ismail Hossain ◽  
M. Abdullah Ansary

2008 ◽  
Vol 47 (11) ◽  
pp. 2960-2965 ◽  
Author(s):  
Hong-Lin Liu ◽  
Zi-Xiang Liu ◽  
Jian-Song Hou ◽  
Shu-Zheng Yang

2009 ◽  
Vol 24 (27) ◽  
pp. 2187-2193 ◽  
Author(s):  
SHU-ZHENG YANG ◽  
KAI LIN ◽  
JUAN YANG

In this paper, the Hawking radiation from the slowly varying nonstationary Reissner–Nordström black hole is discussed through the fermions tunnelling theory, assuming a reasonable form of gamma matrix, and even researching on the issues with following coordinate transformation, which is a new method to study fermions' Hawking tunnelling radiation from slowly varying nonstationary Reissner–Nordström black hole.


2021 ◽  
Vol 2021 (7) ◽  
Author(s):  
Yoshinori Matsuo

Abstract Recently it was proposed that the entanglement entropy of the Hawking radiation contains the information of a region including the interior of the event horizon, which is called “island.” In studies of the entanglement entropy of the Hawking radiation, the total system in the black hole geometry is separated into the Hawking radiation and black hole. In this paper, we study the entanglement entropy of the black hole in the asymptotically flat Schwarzschild spacetime. Consistency with the island rule for the Hawking radiation implies that the information of the black hole is located in a different region than the island. We found an instability of the island in the calculation of the entanglement entropy of the region outside a surface near the horizon. This implies that the region contains all the information of the total system and the information of the black hole is localized on the surface. Thus the surface would be interpreted as the stretched horizon. This structure also resembles black holes in the AdS spacetime with an auxiliary flat spacetime, where the information of the black hole is localized at the interface between the AdS spacetime and the flat spacetime.


2021 ◽  
Vol 2021 (2) ◽  
Author(s):  
Ning Bao ◽  
Yuta Kikuchi

Abstract In the Hayden-Preskill thought experiment, the Hawking radiation emitted before a quantum state is thrown into the black hole is used along with the radiation collected later for the purpose of decoding the quantum state. A natural question is how the recoverability is affected if the stored early radiation is damaged or subject to decoherence, and/or the decoding protocol is imperfectly performed. We study the recoverability in the thought experiment in the presence of decoherence or noise in the storage of early radiation.


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