Absence of the Higuchi bound in a family of alternative linear massive spin-2 models
Autor(a) principal: | |
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Data de Publicação: | 2022 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1088/1361-6382/ac7b06 http://hdl.handle.net/11449/240532 |
Resumo: | There is a well known result from the Fierz-Pauli (FP) theory in de Sitter background, it is the existence of a lower bound for the mass m of the spin 2 particle, the Higuchi bound. It establishes that m 2 ≥ 2H 2, where H is the Hubble parameter, in order to the theory presents no ghost-like instabilities. In this sense, m should be unacceptable high in order to fulfill this condition at the time of the inflationary epoch of the Universe, posing a difficulty to conciliate the FP theory with cosmology. In this article we show that the Higuchi bound can be circumvented in an alternative description of massive spin-2 particles known as L(a1) models. In maximally symmetric spaces the theory has two free parameters which can be consistently chosen in order to make the model absent of a lower bound for m. Then, m can be arbitrarily smaller than the energy scale of inflation avoiding instabilities at that time. |
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Absence of the Higuchi bound in a family of alternative linear massive spin-2 modelsgravitationgravitonHiguchimodified theories of gravityThere is a well known result from the Fierz-Pauli (FP) theory in de Sitter background, it is the existence of a lower bound for the mass m of the spin 2 particle, the Higuchi bound. It establishes that m 2 ≥ 2H 2, where H is the Hubble parameter, in order to the theory presents no ghost-like instabilities. In this sense, m should be unacceptable high in order to fulfill this condition at the time of the inflationary epoch of the Universe, posing a difficulty to conciliate the FP theory with cosmology. In this article we show that the Higuchi bound can be circumvented in an alternative description of massive spin-2 particles known as L(a1) models. In maximally symmetric spaces the theory has two free parameters which can be consistently chosen in order to make the model absent of a lower bound for m. Then, m can be arbitrarily smaller than the energy scale of inflation avoiding instabilities at that time.Divisão de Astrofísica Instituto Nacional de Pesquisas Espaciais, Avenida dos Astronautas 1758, SPUniversidade Estadual Paulista (UNESP) Instituto de Ciência e Tecnologia, SPUniversidade Estadual Paulista (UNESP) Instituto de Ciência e Tecnologia, SPInstituto Nacional de Pesquisas EspaciaisUniversidade Estadual Paulista (UNESP)Fortes, Hemily G. M.Alves, Márcio E. S. [UNESP]2023-03-01T20:21:17Z2023-03-01T20:21:17Z2022-08-04info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1088/1361-6382/ac7b06Classical and Quantum Gravity, v. 39, n. 15, 2022.1361-63820264-9381http://hdl.handle.net/11449/24053210.1088/1361-6382/ac7b062-s2.0-85134797065Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengClassical and Quantum Gravityinfo:eu-repo/semantics/openAccess2023-03-01T20:21:17Zoai:repositorio.unesp.br:11449/240532Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-05-23T20:18:51.086346Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Absence of the Higuchi bound in a family of alternative linear massive spin-2 models |
title |
Absence of the Higuchi bound in a family of alternative linear massive spin-2 models |
spellingShingle |
Absence of the Higuchi bound in a family of alternative linear massive spin-2 models Fortes, Hemily G. M. gravitation graviton Higuchi modified theories of gravity |
title_short |
Absence of the Higuchi bound in a family of alternative linear massive spin-2 models |
title_full |
Absence of the Higuchi bound in a family of alternative linear massive spin-2 models |
title_fullStr |
Absence of the Higuchi bound in a family of alternative linear massive spin-2 models |
title_full_unstemmed |
Absence of the Higuchi bound in a family of alternative linear massive spin-2 models |
title_sort |
Absence of the Higuchi bound in a family of alternative linear massive spin-2 models |
author |
Fortes, Hemily G. M. |
author_facet |
Fortes, Hemily G. M. Alves, Márcio E. S. [UNESP] |
author_role |
author |
author2 |
Alves, Márcio E. S. [UNESP] |
author2_role |
author |
dc.contributor.none.fl_str_mv |
Instituto Nacional de Pesquisas Espaciais Universidade Estadual Paulista (UNESP) |
dc.contributor.author.fl_str_mv |
Fortes, Hemily G. M. Alves, Márcio E. S. [UNESP] |
dc.subject.por.fl_str_mv |
gravitation graviton Higuchi modified theories of gravity |
topic |
gravitation graviton Higuchi modified theories of gravity |
description |
There is a well known result from the Fierz-Pauli (FP) theory in de Sitter background, it is the existence of a lower bound for the mass m of the spin 2 particle, the Higuchi bound. It establishes that m 2 ≥ 2H 2, where H is the Hubble parameter, in order to the theory presents no ghost-like instabilities. In this sense, m should be unacceptable high in order to fulfill this condition at the time of the inflationary epoch of the Universe, posing a difficulty to conciliate the FP theory with cosmology. In this article we show that the Higuchi bound can be circumvented in an alternative description of massive spin-2 particles known as L(a1) models. In maximally symmetric spaces the theory has two free parameters which can be consistently chosen in order to make the model absent of a lower bound for m. Then, m can be arbitrarily smaller than the energy scale of inflation avoiding instabilities at that time. |
publishDate |
2022 |
dc.date.none.fl_str_mv |
2022-08-04 2023-03-01T20:21:17Z 2023-03-01T20:21:17Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1088/1361-6382/ac7b06 Classical and Quantum Gravity, v. 39, n. 15, 2022. 1361-6382 0264-9381 http://hdl.handle.net/11449/240532 10.1088/1361-6382/ac7b06 2-s2.0-85134797065 |
url |
http://dx.doi.org/10.1088/1361-6382/ac7b06 http://hdl.handle.net/11449/240532 |
identifier_str_mv |
Classical and Quantum Gravity, v. 39, n. 15, 2022. 1361-6382 0264-9381 10.1088/1361-6382/ac7b06 2-s2.0-85134797065 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Classical and Quantum Gravity |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1803045662446583808 |