General perturbations in D+1 standard and brane cosmology revisited

Fuente: arXiv
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Hauptverfasser: Delfín, Zoé, Cordero, Rubén, Matos, Tonatiuh, García-Aspeitia, Miguel A.
Format: Preprint
Veröffentlicht: 2023
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author Delfín, Zoé
Cordero, Rubén
Matos, Tonatiuh
García-Aspeitia, Miguel A.
author_facet Delfín, Zoé
Cordero, Rubén
Matos, Tonatiuh
García-Aspeitia, Miguel A.
contents In the present work, we generalize the theory of perturbations in a D + 1 dimensional space-time with cosmological constant, studying scalar, vector and tensor perturbations, as well as its structure in Newtonian and Synchronous gauge. We also show the theory of perturbations in the context of brane cosmology, where branes are embedded in a set of D-spatial dimensions, a temporal dimension, and an additional spatial dimension. In both, standard and brane cosmology an unperturbed spacetime is provided with a Friedmann-Lemaitre-Robertson-Walker metric and arbitrary sectional curvature, the matter content has the shape of a perfect fluid. In addition, we consider the arbitrary sectional curvature, obtaining the respective equations in the Newtonian and Synchronous gauge. We highlight that the results presented in this article can be used to treat brane cosmology with two concentric branes or tackle the σ_{8} tension with a braneworld approach. Finally, as an example of the utility of all the technology presented in this paper, we show an application to the energy ux and the repercussions in the framework of the brane-worlds.
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id arxiv_https___arxiv_org_abs_2302_01338
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publishDate 2023
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spellingShingle General perturbations in D+1 standard and brane cosmology revisited
Delfín, Zoé
Cordero, Rubén
Matos, Tonatiuh
García-Aspeitia, Miguel A.
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
In the present work, we generalize the theory of perturbations in a D + 1 dimensional space-time with cosmological constant, studying scalar, vector and tensor perturbations, as well as its structure in Newtonian and Synchronous gauge. We also show the theory of perturbations in the context of brane cosmology, where branes are embedded in a set of D-spatial dimensions, a temporal dimension, and an additional spatial dimension. In both, standard and brane cosmology an unperturbed spacetime is provided with a Friedmann-Lemaitre-Robertson-Walker metric and arbitrary sectional curvature, the matter content has the shape of a perfect fluid. In addition, we consider the arbitrary sectional curvature, obtaining the respective equations in the Newtonian and Synchronous gauge. We highlight that the results presented in this article can be used to treat brane cosmology with two concentric branes or tackle the σ_{8} tension with a braneworld approach. Finally, as an example of the utility of all the technology presented in this paper, we show an application to the energy ux and the repercussions in the framework of the brane-worlds.
title General perturbations in D+1 standard and brane cosmology revisited
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2302.01338