The impact of particle production on gravitational baryogenesis
Autor(a) principal: | |
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Data de Publicação: | 2016 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1016/j.physletb.2016.10.005 http://hdl.handle.net/11449/169064 |
Resumo: | Baryogenesis driven by curvature effects is investigated by taking into account gravitationally induced particle production in the very early Universe. In our scenario, the baryon asymmetry is generated dynamically during an inflationary epoch powered by ultra-relativistic particles. The adiabatic particle production rate provides both the needed negative pressure to accelerate the radiation dominated Universe and a non-zero chemical potential which distinguishes baryons and anti-baryons thereby producing a baryon asymmetry in agreement with the observed value. Reciprocally, the present day asymmetry may be used to determine the inflationary scale at early times. Successful gravitational baryogenesis is dynamically generated for many different choices of the relevant model parameters. |
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The impact of particle production on gravitational baryogenesisBaryogenesis driven by curvature effects is investigated by taking into account gravitationally induced particle production in the very early Universe. In our scenario, the baryon asymmetry is generated dynamically during an inflationary epoch powered by ultra-relativistic particles. The adiabatic particle production rate provides both the needed negative pressure to accelerate the radiation dominated Universe and a non-zero chemical potential which distinguishes baryons and anti-baryons thereby producing a baryon asymmetry in agreement with the observed value. Reciprocally, the present day asymmetry may be used to determine the inflationary scale at early times. Successful gravitational baryogenesis is dynamically generated for many different choices of the relevant model parameters.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Ministério da Educação e CiênciaDepartamento de Astronomia Universidade de São Paulo, Rua do Matão 1226Department of Physics California State University FresnoICTP South American Institute for Fundamental Research UNESP – Univ. Estadual Paulista, Rua Dr. Bento T. Ferraz 271Institute of Experimental and Theoretical Physics Al-Farabi KazNUICTP South American Institute for Fundamental Research UNESP – Univ. Estadual Paulista, Rua Dr. Bento T. Ferraz 271FAPESP: 11/51676-9CNPq: 3105402014-3CAPES: 88881.068485/2014Universidade de São Paulo (USP)California State University FresnoUniversidade Estadual Paulista (Unesp)Institute of Experimental and Theoretical Physics Al-Farabi KazNULima, J. A.S.Singleton, D. [UNESP]2018-12-11T16:44:11Z2018-12-11T16:44:11Z2016-11-10info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article506-511application/pdfhttp://dx.doi.org/10.1016/j.physletb.2016.10.005Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 762, p. 506-511.0370-2693http://hdl.handle.net/11449/16906410.1016/j.physletb.2016.10.0052-s2.0-849925155332-s2.0-84992515533.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics2,336info:eu-repo/semantics/openAccess2023-12-08T06:18:02Zoai:repositorio.unesp.br:11449/169064Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T19:45:29.280123Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
The impact of particle production on gravitational baryogenesis |
title |
The impact of particle production on gravitational baryogenesis |
spellingShingle |
The impact of particle production on gravitational baryogenesis Lima, J. A.S. |
title_short |
The impact of particle production on gravitational baryogenesis |
title_full |
The impact of particle production on gravitational baryogenesis |
title_fullStr |
The impact of particle production on gravitational baryogenesis |
title_full_unstemmed |
The impact of particle production on gravitational baryogenesis |
title_sort |
The impact of particle production on gravitational baryogenesis |
author |
Lima, J. A.S. |
author_facet |
Lima, J. A.S. Singleton, D. [UNESP] |
author_role |
author |
author2 |
Singleton, D. [UNESP] |
author2_role |
author |
dc.contributor.none.fl_str_mv |
Universidade de São Paulo (USP) California State University Fresno Universidade Estadual Paulista (Unesp) Institute of Experimental and Theoretical Physics Al-Farabi KazNU |
dc.contributor.author.fl_str_mv |
Lima, J. A.S. Singleton, D. [UNESP] |
description |
Baryogenesis driven by curvature effects is investigated by taking into account gravitationally induced particle production in the very early Universe. In our scenario, the baryon asymmetry is generated dynamically during an inflationary epoch powered by ultra-relativistic particles. The adiabatic particle production rate provides both the needed negative pressure to accelerate the radiation dominated Universe and a non-zero chemical potential which distinguishes baryons and anti-baryons thereby producing a baryon asymmetry in agreement with the observed value. Reciprocally, the present day asymmetry may be used to determine the inflationary scale at early times. Successful gravitational baryogenesis is dynamically generated for many different choices of the relevant model parameters. |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-11-10 2018-12-11T16:44:11Z 2018-12-11T16:44:11Z |
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/10.1016/j.physletb.2016.10.005 Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 762, p. 506-511. 0370-2693 http://hdl.handle.net/11449/169064 10.1016/j.physletb.2016.10.005 2-s2.0-84992515533 2-s2.0-84992515533.pdf |
url |
http://dx.doi.org/10.1016/j.physletb.2016.10.005 http://hdl.handle.net/11449/169064 |
identifier_str_mv |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 762, p. 506-511. 0370-2693 10.1016/j.physletb.2016.10.005 2-s2.0-84992515533 2-s2.0-84992515533.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics 2,336 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
506-511 application/pdf |
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_ |
1808129114181206016 |