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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Language: | English |
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Wiley
2016-01-01
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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. |
format | Article |
id | doaj-art-bc2440587f92402e9712a223f36a3891 |
institution | Kabale University |
issn | 1687-7357 1687-7365 |
language | English |
publishDate | 2016-01-01 |
publisher | Wiley |
record_format | Article |
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 |
work_keys_str_mv | AT shhendi frgravitysrainbowanditseinsteincounterpart AT beslampanah frgravitysrainbowanditseinsteincounterpart AT spanahiyan frgravitysrainbowanditseinsteincounterpart AT mmomennia frgravitysrainbowanditseinsteincounterpart |