Remarks on the process γγ→νν̄ in astrophysics

Detalhes bibliográficos
Autor(a) principal: Gregores, E. M. [UNESP]
Data de Publicação: 1995
Outros Autores: Mori, F. [UNESP], Natale, A. A. [UNESP], Novaes, S. F. [UNESP], Spehler, D. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.51.4587
http://hdl.handle.net/11449/224993
Resumo: We discuss the astrophysical consequences of the process γγ→νν̄, when this reaction is mediated by either Majorons or composite neutral leptons, and present the constraints on their coupling coming from stellar energy loss arguments. We also discuss the effect of nuclear absorption when this reaction is mediated by pions, and show that no significant output of energy is provided in this case. Finally, we comment on the importance of these processes in cosmology. © 1995 The American Physical Society.
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spelling Remarks on the process γγ→νν̄ in astrophysicsWe discuss the astrophysical consequences of the process γγ→νν̄, when this reaction is mediated by either Majorons or composite neutral leptons, and present the constraints on their coupling coming from stellar energy loss arguments. We also discuss the effect of nuclear absorption when this reaction is mediated by pions, and show that no significant output of energy is provided in this case. Finally, we comment on the importance of these processes in cosmology. © 1995 The American Physical Society.Instituto de Física Teórica, Universidade Estadual Paulista, Rua Pamplona 145, CEP 01405-900 Sao PauloInstituto de Física Teórica, Universidade Estadual Paulista, Rua Pamplona 145, CEP 01405-900 Sao PauloUniversidade Estadual Paulista (UNESP)Gregores, E. M. [UNESP]Mori, F. [UNESP]Natale, A. A. [UNESP]Novaes, S. F. [UNESP]Spehler, D. [UNESP]2022-04-28T20:34:42Z2022-04-28T20:34:42Z1995-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article4587-4590http://dx.doi.org/10.1103/PhysRevD.51.4587Physical Review D, v. 51, n. 8, p. 4587-4590, 1995.0556-2821http://hdl.handle.net/11449/22499310.1103/PhysRevD.51.45872-s2.0-35949005461Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-28T20:34:42Zoai:repositorio.unesp.br:11449/224993Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462022-04-28T20:34:42Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Remarks on the process γγ→νν̄ in astrophysics
title Remarks on the process γγ→νν̄ in astrophysics
spellingShingle Remarks on the process γγ→νν̄ in astrophysics
Gregores, E. M. [UNESP]
title_short Remarks on the process γγ→νν̄ in astrophysics
title_full Remarks on the process γγ→νν̄ in astrophysics
title_fullStr Remarks on the process γγ→νν̄ in astrophysics
title_full_unstemmed Remarks on the process γγ→νν̄ in astrophysics
title_sort Remarks on the process γγ→νν̄ in astrophysics
author Gregores, E. M. [UNESP]
author_facet Gregores, E. M. [UNESP]
Mori, F. [UNESP]
Natale, A. A. [UNESP]
Novaes, S. F. [UNESP]
Spehler, D. [UNESP]
author_role author
author2 Mori, F. [UNESP]
Natale, A. A. [UNESP]
Novaes, S. F. [UNESP]
Spehler, D. [UNESP]
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
dc.contributor.author.fl_str_mv Gregores, E. M. [UNESP]
Mori, F. [UNESP]
Natale, A. A. [UNESP]
Novaes, S. F. [UNESP]
Spehler, D. [UNESP]
description We discuss the astrophysical consequences of the process γγ→νν̄, when this reaction is mediated by either Majorons or composite neutral leptons, and present the constraints on their coupling coming from stellar energy loss arguments. We also discuss the effect of nuclear absorption when this reaction is mediated by pions, and show that no significant output of energy is provided in this case. Finally, we comment on the importance of these processes in cosmology. © 1995 The American Physical Society.
publishDate 1995
dc.date.none.fl_str_mv 1995-01-01
2022-04-28T20:34:42Z
2022-04-28T20:34:42Z
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/10.1103/PhysRevD.51.4587
Physical Review D, v. 51, n. 8, p. 4587-4590, 1995.
0556-2821
http://hdl.handle.net/11449/224993
10.1103/PhysRevD.51.4587
2-s2.0-35949005461
url http://dx.doi.org/10.1103/PhysRevD.51.4587
http://hdl.handle.net/11449/224993
identifier_str_mv Physical Review D, v. 51, n. 8, p. 4587-4590, 1995.
0556-2821
10.1103/PhysRevD.51.4587
2-s2.0-35949005461
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 4587-4590
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
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