Planck scale effects on the thermodynamics of photon gases

Mir Mehedi Faruk and Md. Muktadir Rahman
Phys. Rev. D 94, 105018 – Published 18 November 2016

Abstract

A particular framework for quantum gravity is the doubly special relativity formalism that introduces a new observer-independent scale (the Planck scale). We resort to the methods of statistical mechanics in this framework to determine how the deformed dispersion relation affects the thermodynamics of a photon gas. The ensuing modifications to the density of states, partition function, pressure, internal energy, entropy, free energy, and specific heat are calculated. These results are compared with the outcome obtained in the Lorentz violating model of Camacho and Marcias [Gen. Relativ. Gravit. 39, 1175 (2007)]. The two types of models predict different results due to different spacetime structures near the Planck scale. The resulting modifications can be interpreted as a consequence of the deformed Lorentz symmetry present in the particular model we have considered. In the low energy limit, our calculation coincides with the usual results of photon thermodynamics in special relativity theory, in contrast to the study presented in an earlier article [Phys. Rev. D 81, 085039 (2010)].

  • Figure
  • Figure
  • Received 26 May 2016

DOI:https://doi.org/10.1103/PhysRevD.94.105018

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Mir Mehedi Faruk*

  • Theoretical Physics, Blackett Laboratory, Imperial College, London SW7 2AZ, United Kingdom

Md. Muktadir Rahman

  • Department of Theoretical Physics, University of Dhaka, Dhaka-1000, Bangladesh

  • *mir.faruk15@imperial.ac.uk mir.mehedi.faruk@cern.ch
  • muturza3.1416@gmail.com

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Issue

Vol. 94, Iss. 10 — 15 November 2016

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