Phase transition of charged Black Holes in Brans–Dicke theory through geometrical thermodynamics

In this paper, we take into account black hole solutions of Brans–Dicke–Maxwell theory and investigate their stability and phase transition points. We apply the concept of geometry in thermodynamics to obtain phase transition points and compare its results with those, calculated in the canonical ens...

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Published in:The European physical journal. C, Particles and fields Vol. 76; no. 7; p. 1
Main Authors: Hendi, S. H., Panahiyan, S., Panah, B. Eslam, Armanfard, Z.
Format: Journal Article
Language:English
Published: Berlin/Heidelberg Springer Berlin Heidelberg 13-07-2016
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Abstract In this paper, we take into account black hole solutions of Brans–Dicke–Maxwell theory and investigate their stability and phase transition points. We apply the concept of geometry in thermodynamics to obtain phase transition points and compare its results with those, calculated in the canonical ensemble through heat capacity. We show that these black holes enjoy second order phase transitions. We also show that there is a lower bound for the horizon radius of physical charged black holes in Brans–Dicke theory, which originates from restrictions of positivity of temperature. In addition, we find that employing a specific thermodynamical metric in the context of geometrical thermodynamics yields divergencies for the thermodynamical Ricci scalar in places of the phase transitions. It will be pointed out that due to the characteristic behavior of the thermodynamical Ricci scalar around its divergence points, one is able to distinguish the physical limitation point from the phase transitions. In addition, the free energy of these black holes will be obtained and its behavior will be investigated. It will be shown that the behavior of the free energy in the place where the heat capacity diverges demonstrates second order phase transition characteristics.
AbstractList In this paper, we take into account black hole solutions of Brans-Dicke-Maxwell theory and investigate their stability and phase transition points. We apply the concept of geometry in thermodynamics to obtain phase transition points and compare its results with those, calculated in the canonical ensemble through heat capacity. We show that these black holes enjoy second order phase transitions. We also show that there is a lower bound for the horizon radius of physical charged black holes in Brans-Dicke theory, which originates from restrictions of positivity of temperature. In addition, we find that employing a specific thermodynamical metric in the context of geometrical thermodynamics yields divergencies for the thermodynamical Ricci scalar in places of the phase transitions. It will be pointed out that due to the characteristic behavior of the thermodynamical Ricci scalar around its divergence points, one is able to distinguish the physical limitation point from the phase transitions. In addition, the free energy of these black holes will be obtained and its behavior will be investigated. It will be shown that the behavior of the free energy in the place where the heat capacity diverges demonstrates second order phase transition characteristics.
ArticleNumber 396
Audience Academic
Author Armanfard, Z.
Panah, B. Eslam
Hendi, S. H.
Panahiyan, S.
Author_xml – sequence: 1
  givenname: S. H.
  orcidid: 0000-0002-4444-6579
  surname: Hendi
  fullname: Hendi, S. H.
  email: hendi@shirazu.ac.ir
  organization: Physics Department and Biruni Observatory, College of Sciences, Shiraz University, Research Institute for Astronomy and Astrophysics of Maragha (RIAAM)
– sequence: 2
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  surname: Panahiyan
  fullname: Panahiyan, S.
  organization: Physics Department and Biruni Observatory, College of Sciences, Shiraz University, Physics Department, Shahid Beheshti University
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  givenname: B. Eslam
  surname: Panah
  fullname: Panah, B. Eslam
  organization: Physics Department and Biruni Observatory, College of Sciences, Shiraz University
– sequence: 4
  givenname: Z.
  surname: Armanfard
  fullname: Armanfard, Z.
  organization: Physics Department and Biruni Observatory, College of Sciences, Shiraz University
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Keywords Black Hole Solution
Order Phase Transition
Black Hole
Heat Capacity
Divergence Point
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SSID ssj0002408
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Snippet In this paper, we take into account black hole solutions of Brans–Dicke–Maxwell theory and investigate their stability and phase transition points. We apply...
In this paper, we take into account black hole solutions of Brans-Dicke-Maxwell theory and investigate their stability and phase transition points. We apply...
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SubjectTerms Analysis
Astronomy
Astrophysics and Cosmology
Black holes
Elementary Particles
Hadrons
Heavy Ions
Measurement Science and Instrumentation
Nuclear Energy
Nuclear Physics
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Regular Article - Theoretical Physics
String Theory
Thermodynamics
Title Phase transition of charged Black Holes in Brans–Dicke theory through geometrical thermodynamics
URI https://link.springer.com/article/10.1140/epjc/s10052-016-4235-1
https://www.proquest.com/docview/1846959193
Volume 76
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