Multi-field TDiff theories for cosmology
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 (...
| Autores: | , , |
|---|---|
| Tipo de recurso: | artículo |
| Fecha de publicación: | 2025 |
| País: | España |
| Institución: | Universidad Complutense de Madrid (UCM) |
| Repositorio: | Docta Complutense |
| Idioma: | inglés |
| OAI Identifier: | oai:docta.ucm.es:20.500.14352/128414 |
| Acceso en línea: | https://hdl.handle.net/20.500.14352/128414 |
| Access Level: | acceso abierto |
| Palabra clave: | 53 524.8 530.145 Cosmology Scalar fields Shift-symmetry Transverse diffeomorphisms Dark energy Interacting dark sector Física (Física) Teoría de los quanta 2212 Física Teórica 2101 Cosmología y Cosmogonía 2212.14 Teoría de la Relatividad |
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Multi-field TDiff theories for cosmologyTessainer, DiegoLópez Maroto, AntonioMartín Moruno, María Del Prado53524.8530.145CosmologyScalar fieldsShift-symmetryTransverse diffeomorphismsDark energyInteracting dark sectorFísica (Física)Teoría de los quanta2212 Física Teórica2101 Cosmología y Cosmogonía2212.14 Teoría de la RelatividadWe 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.ElsevierUniversidad Complutense de Madrid20252025-02-0120252025-02-01journal articlehttp://purl.org/coar/resource_type/c_6501VoRhttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/20.500.14352/128414reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)InglésengAgencia Estatal de Investigación http://dx.doi.org/10.13039/501100011033 Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023 PID2022-138263NB-I00 COSMOLOGIA Y GRAVITACION DEL SECTOR OSCUROopen accesshttp://purl.org/coar/access_right/c_abf2Attribution 4.0 Internationalhttp://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/1284142026-06-02T12:44:21Z |
| dc.title.none.fl_str_mv |
Multi-field TDiff theories for cosmology |
| title |
Multi-field TDiff theories for cosmology |
| spellingShingle |
Multi-field TDiff theories for cosmology Tessainer, Diego 53 524.8 530.145 Cosmology Scalar fields Shift-symmetry Transverse diffeomorphisms Dark energy Interacting dark sector Física (Física) Teoría de los quanta 2212 Física Teórica 2101 Cosmología y Cosmogonía 2212.14 Teoría de la Relatividad |
| title_short |
Multi-field TDiff theories for cosmology |
| title_full |
Multi-field TDiff theories for cosmology |
| title_fullStr |
Multi-field TDiff theories for cosmology |
| title_full_unstemmed |
Multi-field TDiff theories for cosmology |
| title_sort |
Multi-field TDiff theories for cosmology |
| dc.creator.none.fl_str_mv |
Tessainer, Diego López Maroto, Antonio Martín Moruno, María Del Prado |
| author |
Tessainer, Diego |
| author_facet |
Tessainer, Diego López Maroto, Antonio Martín Moruno, María Del Prado |
| author_role |
author |
| author2 |
López Maroto, Antonio Martín Moruno, María Del Prado |
| author2_role |
author author |
| dc.contributor.none.fl_str_mv |
Universidad Complutense de Madrid |
| dc.subject.none.fl_str_mv |
53 524.8 530.145 Cosmology Scalar fields Shift-symmetry Transverse diffeomorphisms Dark energy Interacting dark sector Física (Física) Teoría de los quanta 2212 Física Teórica 2101 Cosmología y Cosmogonía 2212.14 Teoría de la Relatividad |
| topic |
53 524.8 530.145 Cosmology Scalar fields Shift-symmetry Transverse diffeomorphisms Dark energy Interacting dark sector Física (Física) Teoría de los quanta 2212 Física Teórica 2101 Cosmología y Cosmogonía 2212.14 Teoría de la Relatividad |
| description |
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. |
| publishDate |
2025 |
| dc.date.none.fl_str_mv |
2025 2025-02-01 2025 2025-02-01 |
| dc.type.none.fl_str_mv |
journal article http://purl.org/coar/resource_type/c_6501 VoR http://purl.org/coar/version/c_970fb48d4fbd8a85 |
| dc.type.openaire.fl_str_mv |
info:eu-repo/semantics/article |
| format |
article |
| dc.identifier.none.fl_str_mv |
https://hdl.handle.net/20.500.14352/128414 |
| url |
https://hdl.handle.net/20.500.14352/128414 |
| dc.language.none.fl_str_mv |
Inglés eng |
| language_invalid_str_mv |
Inglés |
| language |
eng |
| dc.relation.none.fl_str_mv |
Agencia Estatal de Investigación http://dx.doi.org/10.13039/501100011033 Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023 PID2022-138263NB-I00 COSMOLOGIA Y GRAVITACION DEL SECTOR OSCURO |
| dc.rights.none.fl_str_mv |
open access http://purl.org/coar/access_right/c_abf2 Attribution 4.0 International http://creativecommons.org/licenses/by/4.0/ |
| dc.rights.openaire.fl_str_mv |
info:eu-repo/semantics/openAccess |
| rights_invalid_str_mv |
open access http://purl.org/coar/access_right/c_abf2 Attribution 4.0 International http://creativecommons.org/licenses/by/4.0/ |
| eu_rights_str_mv |
openAccess |
| dc.format.none.fl_str_mv |
application/pdf |
| dc.publisher.none.fl_str_mv |
Elsevier |
| publisher.none.fl_str_mv |
Elsevier |
| dc.source.none.fl_str_mv |
reponame:Docta Complutense instname:Universidad Complutense de Madrid (UCM) |
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Universidad Complutense de Madrid (UCM) |
| reponame_str |
Docta Complutense |
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Docta Complutense |
| repository.name.fl_str_mv |
|
| repository.mail.fl_str_mv |
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15,812429 |