Quantum thermodynamics of an α'-corrected Reissner-Nordstrom black hole

被引:8
|
作者
Pourhassan, Behnam [1 ,2 ,5 ]
Sakalli, Izzet [3 ]
Shi, Xiaoping [4 ]
Faizal, Mir [4 ,5 ]
Wani, Salman Sajad [6 ]
机构
[1] Damghan Univ, Sch Phys, Damghan 3671641167, Iran
[2] Istanbul Tech Univ, Phys Dept, TR-34469 Istanbul, Turkiye
[3] Eastern Mediterranean Univ, Phys Dept, Via Mersin 10, TR-99628 Famagusta, North Cyprus, Turkiye
[4] Univ British Columbia Okanagan, Irving K Barber Sch Arts & Sci, Kelowna, BC V1V 1V7, Canada
[5] Canadian Quantum Res Ctr, 204-3002 32 Ave, Vernon, BC V1T 2L7, Canada
[6] Istanbul Tech Univ, Dept Phys Engn, TR-34469 Istanbul, Turkiye
基金
加拿大自然科学与工程研究理事会;
关键词
ZERO-POINT LENGTH; HOLOGRAPHIC PRINCIPLE; ENTROPY; DUALITY;
D O I
10.1209/0295-5075/acfff0
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In this paper, we will go beyond equilibrium description to properly investigate the evaporation of a Reissner-Nordstro center dot m black hole. Thus, we will explicitly apply techniques of non-equilibrium quantum thermodynamics to this black hole. As the non-equilibrium effects would become important at the quantum scale, we will incorporate the quantum gravitational corrections by using an alpha'-corrected Reissner-Nordstro center dot m black hole. We will start by developing a novel alpha'-corrected first law. Then we will investigate the quantum gravitational corrections to the Parikh-Wilczek formalism, and introduce Kullback-Leibler divergence to quantify the effects of corrections. Furthermore, we will demonstrate that the non-thermal nature of radiation in the Parikh-Wilczek formalism can be directly related to the average quantum work done on the emitted particles using non-equilibrium quantum thermodynamics. This is because the average quantum work done is a unitary process in non-equilibrium quantum thermodynamics. We will use the Ramsey scheme for emitted particles to calculate this quantum work distribution for the emitted particles.
引用
收藏
页数:8
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