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Modified Gravity: From Black Holes Entropy to Current Cosmology II

A special issue of Entropy (ISSN 1099-4300). This special issue belongs to the section "Astrophysics, Cosmology, and Black Holes".

Deadline for manuscript submissions: closed (31 May 2019) | Viewed by 9948

Special Issue Editors


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Instituto de Ciencias del Espacio (ICE), Consejo Superior de Investigaciones Científicas (CSIC) and Institut d'Estudis Espacials de Catalunya (IEEC), Campus UAB, Carrer de Can Magrans s/n, 08193 Bellaterra (Barcelona), Spain
Interests: theoretical cosmology; dark energy; modified gravity; inflation
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Guest Editor
Instituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências da Universidade de Lisboa, Edifício C8, Campo Grande, P-1749-016 Lisbon, Portugal
Interests: black holes; modified gravity; cosmology; bouncing solutions; spacetime singularities; nonlinear electrodynamics; field theory; topological defects; metric-affine geometry
Special Issues, Collections and Topics in MDPI journals

Special Issue Information

Dear Colleagues,

Cosmology is experiencing its golden era, when more and more data, released by current and future missions, is providing a way to test cosmological models with a high precision. As pointed by the observations from the last decade, the current expansion of the universe is being accelerated, due to the presence of an unknown fluid, which behaves effectively as a perfect fluid with negative pressure and which has been called dark energy. Such a fluid raises fundamental thermodynamical issues that are unknown or at least not yet well understood. Dark energy entropy, its specific heat or how (non)-adiabatic perturbations may be affected by each dark energy model are topics to be considered in this Special Issue. Additionally, possible interactions among dark energy and dark matter may affect the thermodynamics of both unknown components. Moreover, the thermodynamics of the early universe, particularly along and at the end of the inflationary period, have been deeply studied and required special analyses, which can contribute to a better understanding of the universe evolution.

On the other hand, since the establishment of the fundamental connection between gravitation and standard thermodynamic systems following Hawking’s temperature and Bekenstein’s area law, the study of black hole thermodynamics has become one of the most promising scenarios to test our comprehension of gravitational interaction in combination with quantum effects. The consideration of modified theories of gravity offer new scenarios regarding, among many others, the definition of black hole entropy, the validity of the second law, the existence of different kinds of phase transitions, the description of the last stages of black hole evaporation, or the resolution of the information loss problem.

This Special Issue is devoted to discuss the latest achievements on the understanding of the thermodynamics of gravitational physics and cosmology, and particularly on those theories beyond General Relativity. We expect that this Special Issue can account for new physics regarding properties of dark energy and its alternatives, as well as new insights on the thermodynamical properties of gravitational systems such as black holes or wormholes.

Dr. Diego Sáez-Chillón Gómez
Dr. Diego Rubiera-Garcia
Guest Editors

Manuscript Submission Information

Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 100 words) can be sent to the Editorial Office for announcement on this website.

Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Entropy is an international peer-reviewed open access monthly journal published by MDPI.

Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 2600 CHF (Swiss Francs). Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.

Keywords

  • Quantum aspects of black holes: thermodynamics, evaporation, phase transitions
  • Black hole entropy
  • Modified theories of gravity
  • Cosmology
  • Dark energy
  • Inflation

Published Papers (3 papers)

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Research

9 pages, 284 KiB  
Article
Non-Geodesic Incompleteness in Poincaré Gauge Gravity
by José Alberto Ruiz Cembranos, Jorge Gigante Valcarcel and Francisco J. Maldonado Torralba
Entropy 2019, 21(3), 280; https://doi.org/10.3390/e21030280 - 14 Mar 2019
Cited by 6 | Viewed by 2601
Abstract
In this work, we review the study of singularities in Poincaré gauge theories of gravity. Since one of the most recent studies used the appearance of black hole regions of arbitrary dimension as an indicator of singular behavior, we also give some explicit [...] Read more.
In this work, we review the study of singularities in Poincaré gauge theories of gravity. Since one of the most recent studies used the appearance of black hole regions of arbitrary dimension as an indicator of singular behavior, we also give some explicit examples of these structures and study how particles behave around them. Full article
(This article belongs to the Special Issue Modified Gravity: From Black Holes Entropy to Current Cosmology II)
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16 pages, 303 KiB  
Article
Thermodynamics of f(R) Gravity with Disformal Transformation
by Chao-Qiang Geng, Wei-Cheng Hsu, Jhih-Rong Lu and Ling-Wei Luo
Entropy 2019, 21(2), 172; https://doi.org/10.3390/e21020172 - 13 Feb 2019
Cited by 6 | Viewed by 2514
Abstract
We study thermodynamics in f ( R ) gravity with the disformal transformation. The transformation applied to the matter Lagrangian has the form of [...] Read more.
We study thermodynamics in f ( R ) gravity with the disformal transformation. The transformation applied to the matter Lagrangian has the form of γ μ ν = A ( ϕ , X ) g μ ν + B ( ϕ , X ) μ ϕ ν ϕ with the assumption of the Minkowski matter metric γ μ ν = η μ ν , where ϕ is the disformal scalar and X is the corresponding kinetic term of ϕ . We verify the generalized first and second laws of thermodynamics in this disformal type of f ( R ) gravity in the Friedmann-Lemaître-Robertson-Walker (FLRW) universe. In addition, we show that the Hubble parameter contains the disformally induced terms, which define the effectively varying equations of state for matter. Full article
(This article belongs to the Special Issue Modified Gravity: From Black Holes Entropy to Current Cosmology II)
10 pages, 782 KiB  
Article
Thermodynamics in the Universe Described by the Emergence of Space and the Energy Balance Relation
by Fei-Quan Tu, Yi-Xin Chen and Qi-Hong Huang
Entropy 2019, 21(2), 167; https://doi.org/10.3390/e21020167 - 11 Feb 2019
Cited by 7 | Viewed by 4258
Abstract
It has previously been shown that it is more common to describe the evolution of the universe based on the emergence of space and the energy balance relation. Here we investigate the thermodynamic properties of the universe described by such a model. We [...] Read more.
It has previously been shown that it is more common to describe the evolution of the universe based on the emergence of space and the energy balance relation. Here we investigate the thermodynamic properties of the universe described by such a model. We show that the first law of thermodynamics and the generalized second law of thermodynamics (GSLT) are both satisfied and the weak energy condition are also fulfilled for two typical examples. Finally, we examine the physical consistency for the present model. The results show that there exists a good thermodynamic description for such a universe. Full article
(This article belongs to the Special Issue Modified Gravity: From Black Holes Entropy to Current Cosmology II)
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