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Entropy 2015, 17(4), 1549-1557; doi:10.3390/e17041549

Thermodynamics in Curved Space-Time and Its Application to Holography

College of Physical Science and Technology, Hebei University, Baoding 071002, China
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Authors to whom correspondence should be addressed.
Academic Editors: Kazuharu Bamba and Oleg Lunin
Received: 8 January 2015 / Revised: 12 March 2015 / Accepted: 18 March 2015 / Published: 24 March 2015
(This article belongs to the Special Issue Holographic Principle and Its Application)
View Full-Text   |   Download PDF [191 KB, uploaded 24 March 2015]

Abstract

The thermodynamic behaviors of a system living in a curved space-time are different from those of a system in a flat space-time. We have investigated the thermodynamics for a system consisting of relativistic massless bosons. We show that a strongly curved metric will produce a large enhancement of the degrees of freedom in the formulae of energy and entropy of the system, as a comparison to the case in a flat space-time. We are mainly concerned with its implications to holography, including the derivations of holographic entropy and holographic screen. View Full-Text
Keywords: black hole; holographic principle; entropy bounds black hole; holographic principle; entropy bounds
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (CC BY 4.0).

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MDPI and ACS Style

Xiao, Y.; Feng, L.-H.; Guan, L. Thermodynamics in Curved Space-Time and Its Application to Holography. Entropy 2015, 17, 1549-1557.

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