Absence of the Higuchi bound in a family of alternative linear massive spin-2 models

Detalhes bibliográficos
Autor(a) principal: Fortes, Hemily G. M.
Data de Publicação: 2022
Outros Autores: Alves, Márcio E. S. [UNESP]
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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spelling 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)
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