Multi-field TDiff theories for cosmology

Fuente: arXiv
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Main Authors: Tessainer, Diego, Maroto, Antonio L., Martín-Moruno, Prado
Format: Preprint
Published: 2024
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author Tessainer, Diego
Maroto, Antonio L.
Martín-Moruno, Prado
author_facet Tessainer, Diego
Maroto, Antonio L.
Martín-Moruno, Prado
contents We consider theories which break the invariance under diffeomorphisms (Diff) down to transverse diffeomorphisms (TDiff) in the matter sector, consisting of multiple scalar fields. In particular, we regard shift-symmetric models with two free TDiff scalar fields in a flat Robertson-Walker spacetime (FLRW) and use the perfect fluid approach to study their dynamics. As a consequence of the symmetry breaking, an effective interaction between the fields is induced from the conservation of the total energy-momentum tensor, without the necessity to introduce any explicit interacting term in the Lagrangian. We study the different single-field domination regimes and analyze the energy exchange between the fields. Thereupon, we introduce an application of these models for the description of interactions in the dark sector, and compare the theoretical predictions of our model to observational data from Type Ia supernovae.
format Preprint
id arxiv_https___arxiv_org_abs_2409_11991
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Multi-field TDiff theories for cosmology
Tessainer, Diego
Maroto, Antonio L.
Martín-Moruno, Prado
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
We consider theories which break the invariance under diffeomorphisms (Diff) down to transverse diffeomorphisms (TDiff) in the matter sector, consisting of multiple scalar fields. In particular, we regard shift-symmetric models with two free TDiff scalar fields in a flat Robertson-Walker spacetime (FLRW) and use the perfect fluid approach to study their dynamics. As a consequence of the symmetry breaking, an effective interaction between the fields is induced from the conservation of the total energy-momentum tensor, without the necessity to introduce any explicit interacting term in the Lagrangian. We study the different single-field domination regimes and analyze the energy exchange between the fields. Thereupon, we introduce an application of these models for the description of interactions in the dark sector, and compare the theoretical predictions of our model to observational data from Type Ia supernovae.
title Multi-field TDiff theories for cosmology
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2409.11991