The Entropy Inside a Charged Black Hole Under Hawking Radiation

Christodoulou and Rovelli have revealed that black holes have big interiors that grow asymptotically linearly with advanced time. Even if the Hawking radiation is taken into account, such interiors remain large. Based on these findings, we investigate the relation between the entropy contained in th...

Full description

Saved in:
Bibliographic Details
Published in:International journal of theoretical physics 2018-11, Vol.57 (11), p.3429-3435
Main Authors: Han, Shan-Zhong, Yang, Jian-Zhi, Wang, Xin-Yang, Liu, Wen-Biao
Format: Article
Language:English
Subjects:
Black holes
Elementary Particles
Entropy
Hawking radiation
Mathematical and Computational Physics
Physics
Physics and Astronomy
Quantum Field Theory
Quantum Physics
Theoretical
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Christodoulou and Rovelli have revealed that black holes have big interiors that grow asymptotically linearly with advanced time. Even if the Hawking radiation is taken into account, such interiors remain large. Based on these findings, we investigate the relation between the entropy contained in the maximum interior volume of a charged black hole and the Bekenstein-Hawking entropy using an improved method. We find that, in the early stages of the radiation, the variation of the entropy is proportional to the variation of the Bekenstein-Hawking entropy. As the radiation progresses, the magnitude of the ratio will be gradually decreasing
ISSN:0020-7748
1572-9575
DOI:10.1007/s10773-018-3856-6