F(R) Gravity’s Rainbow and Its Einstein Counterpart

Motivated by UV completion of general relativity with a modification of a geometry at high energy scale, it is expected to have an energy dependent geometry. In this paper, we introduce charged black hole solutions with power Maxwell invariant source in the context of gravity’s rainbow. In addition,...

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Main Authors: S. H. Hendi, B. Eslam Panah, S. Panahiyan, M. Momennia
Format: Article
Language:English
Published: Wiley 2016-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2016/9813582
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author S. H. Hendi
B. Eslam Panah
S. Panahiyan
M. Momennia
author_facet S. H. Hendi
B. Eslam Panah
S. Panahiyan
M. Momennia
author_sort S. H. Hendi
collection DOAJ
description Motivated by UV completion of general relativity with a modification of a geometry at high energy scale, it is expected to have an energy dependent geometry. In this paper, we introduce charged black hole solutions with power Maxwell invariant source in the context of gravity’s rainbow. In addition, we investigate two classes of F(R) gravity’s rainbow solutions. At first, we study energy dependent F(R) gravity without energy-momentum tensor, and then we obtain F(R) gravity’s rainbow in the presence of conformally invariant Maxwell source. We study geometrical properties of the mentioned solutions and compare their results. We also give some related comments regarding thermodynamical behavior of the obtained solutions and discuss thermal stability of the solutions.
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institution Kabale University
issn 1687-7357
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publishDate 2016-01-01
publisher Wiley
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series Advances in High Energy Physics
spelling doaj-art-bc2440587f92402e9712a223f36a38912025-02-03T05:51:32ZengWileyAdvances in High Energy Physics1687-73571687-73652016-01-01201610.1155/2016/98135829813582F(R) Gravity’s Rainbow and Its Einstein CounterpartS. H. Hendi0B. Eslam Panah1S. Panahiyan2M. Momennia3Physics Department and Biruni Observatory, College of Sciences, Shiraz University, Shiraz 71454, IranPhysics Department and Biruni Observatory, College of Sciences, Shiraz University, Shiraz 71454, IranPhysics Department and Biruni Observatory, College of Sciences, Shiraz University, Shiraz 71454, IranPhysics Department and Biruni Observatory, College of Sciences, Shiraz University, Shiraz 71454, IranMotivated by UV completion of general relativity with a modification of a geometry at high energy scale, it is expected to have an energy dependent geometry. In this paper, we introduce charged black hole solutions with power Maxwell invariant source in the context of gravity’s rainbow. In addition, we investigate two classes of F(R) gravity’s rainbow solutions. At first, we study energy dependent F(R) gravity without energy-momentum tensor, and then we obtain F(R) gravity’s rainbow in the presence of conformally invariant Maxwell source. We study geometrical properties of the mentioned solutions and compare their results. We also give some related comments regarding thermodynamical behavior of the obtained solutions and discuss thermal stability of the solutions.http://dx.doi.org/10.1155/2016/9813582
spellingShingle S. H. Hendi
B. Eslam Panah
S. Panahiyan
M. Momennia
F(R) Gravity’s Rainbow and Its Einstein Counterpart
Advances in High Energy Physics
title F(R) Gravity’s Rainbow and Its Einstein Counterpart
title_full F(R) Gravity’s Rainbow and Its Einstein Counterpart
title_fullStr F(R) Gravity’s Rainbow and Its Einstein Counterpart
title_full_unstemmed F(R) Gravity’s Rainbow and Its Einstein Counterpart
title_short F(R) Gravity’s Rainbow and Its Einstein Counterpart
title_sort f r gravity s rainbow and its einstein counterpart
url http://dx.doi.org/10.1155/2016/9813582
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AT beslampanah frgravitysrainbowanditseinsteincounterpart
AT spanahiyan frgravitysrainbowanditseinsteincounterpart
AT mmomennia frgravitysrainbowanditseinsteincounterpart