AdS 4 dyonic black holes in gravity's rainbow

Panahiyan, S.  (Helmholtz-Institut Jena, Fröbelstieg 3, Jena, D-07743, Germany) (GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, D-64291, Germany) (Theoretisch-Physikalisches Institut, Friedrich-Schiller-University Jena, Jena, D-07743, Germany) ; Hendi, S.H.  (Physics Department, Biruni Observatory, College of Sciences, Shiraz University, Shiraz, 71454, Iran) (Research Institute for Astronomy and Astrophysics of Maragha (RIAAM), P.O. Box 55134-441, Maragha, Iran) ; Riazi, N. (Physics Department, Shahid Beheshti University, Tehran, 19839, Iran)

27 November 2018

Abstract: In this paper, we investigate thermodynamical structure of dyonic black holes in the presence of gravity's rainbow. We confirm that for super magnetized and highly pressurized scenarios, the number of black holes' phases is reduced to a single phase. In addition, due to specific coupling of rainbow functions, it is possible to track the effects of temporal and spatial parts of our setup on thermodynamical quantities/behaviors including equilibrium point, existence of multiple phases, possible phase transitions and conditions for having a uniform stable structure.

Published in: Nuclear Physics B 938 (2019) 388-415
Published by: Elsevier
DOI: 10.1016/j.nuclphysb.2018.11.019
License: CC-BY-3.0

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