Cosmological perturbations in modified teleparallel gravity models: boundary term extension
Abstract Teleparallel gravity offers a new avenue in which to construct gravitational models beyond general relativity. While teleparallel gravity can be framed in a way to be dynamically equivalent to general relativity, its modifications are mostly not equivalent to the traditional route to modifi...
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Series: | European Physical Journal C: Particles and Fields |
Online Access: | https://doi.org/10.1140/epjc/s10052-021-08833-2 |
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doaj-4b1e73509463489f9cc8b7308a9c224d2021-01-24T12:40:51ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522021-01-0181111610.1140/epjc/s10052-021-08833-2Cosmological perturbations in modified teleparallel gravity models: boundary term extensionSebastian Bahamonde0Viktor Gakis1Stella Kiorpelidi2Tomi Koivisto3Jackson Levi Said4Emmanuel N. Saridakis5Laboratory of Theoretical Physics, Institute of Physics, University of TartuInstitute of Space Sciences and Astronomy, University of MaltaDepartment of Physics, National Technical University of AthensLaboratory of Theoretical Physics, Institute of Physics, University of TartuInstitute of Space Sciences and Astronomy, University of MaltaDepartment of Physics, National Technical University of AthensAbstract Teleparallel gravity offers a new avenue in which to construct gravitational models beyond general relativity. While teleparallel gravity can be framed in a way to be dynamically equivalent to general relativity, its modifications are mostly not equivalent to the traditional route to modified gravity. f(T, B) gravity is one such gravitational theory where the second and fourth order contributions to the field equations are decoupled. In this work, we explore the all important cosmological perturbations of this new framework of gravity. We derive the gravitational propagation equation, its vector perturbation stability conditions, and its scalar perturbations. Together with the matter perturbations, we derive the effective gravitational constant in this framework, and find an interesting branching behaviour that depends on the particular gravitational models being probed. We close with a discussion on the relation of these results with other gravitational theories.https://doi.org/10.1140/epjc/s10052-021-08833-2 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Sebastian Bahamonde Viktor Gakis Stella Kiorpelidi Tomi Koivisto Jackson Levi Said Emmanuel N. Saridakis |
spellingShingle |
Sebastian Bahamonde Viktor Gakis Stella Kiorpelidi Tomi Koivisto Jackson Levi Said Emmanuel N. Saridakis Cosmological perturbations in modified teleparallel gravity models: boundary term extension European Physical Journal C: Particles and Fields |
author_facet |
Sebastian Bahamonde Viktor Gakis Stella Kiorpelidi Tomi Koivisto Jackson Levi Said Emmanuel N. Saridakis |
author_sort |
Sebastian Bahamonde |
title |
Cosmological perturbations in modified teleparallel gravity models: boundary term extension |
title_short |
Cosmological perturbations in modified teleparallel gravity models: boundary term extension |
title_full |
Cosmological perturbations in modified teleparallel gravity models: boundary term extension |
title_fullStr |
Cosmological perturbations in modified teleparallel gravity models: boundary term extension |
title_full_unstemmed |
Cosmological perturbations in modified teleparallel gravity models: boundary term extension |
title_sort |
cosmological perturbations in modified teleparallel gravity models: boundary term extension |
publisher |
SpringerOpen |
series |
European Physical Journal C: Particles and Fields |
issn |
1434-6044 1434-6052 |
publishDate |
2021-01-01 |
description |
Abstract Teleparallel gravity offers a new avenue in which to construct gravitational models beyond general relativity. While teleparallel gravity can be framed in a way to be dynamically equivalent to general relativity, its modifications are mostly not equivalent to the traditional route to modified gravity. f(T, B) gravity is one such gravitational theory where the second and fourth order contributions to the field equations are decoupled. In this work, we explore the all important cosmological perturbations of this new framework of gravity. We derive the gravitational propagation equation, its vector perturbation stability conditions, and its scalar perturbations. Together with the matter perturbations, we derive the effective gravitational constant in this framework, and find an interesting branching behaviour that depends on the particular gravitational models being probed. We close with a discussion on the relation of these results with other gravitational theories. |
url |
https://doi.org/10.1140/epjc/s10052-021-08833-2 |
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