Lasting recombination and cosmic background radiation spectrum

Detalhes bibliográficos
Autor(a) principal: Aldrovandi, R.
Data de Publicação: 1976
Outros Autores: D'Olival, J. B.S.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1007/BF00642533
http://hdl.handle.net/11449/231038
Resumo: The thermal decoupling during recombination and the endurance of this process can significantly deform the black-body background radiation spectrum even in the absence of heating sources. Observational data contradicts a flat standard universe but agrees with a low-density model and with a flat matter-antimatter symmetric universe. Evidence is presented against the presumption that matter-antimatter annibilation should necessarily produce large distortions. © 1976 D. Reidel Publishing Company.
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spelling Lasting recombination and cosmic background radiation spectrumThe thermal decoupling during recombination and the endurance of this process can significantly deform the black-body background radiation spectrum even in the absence of heating sources. Observational data contradicts a flat standard universe but agrees with a low-density model and with a flat matter-antimatter symmetric universe. Evidence is presented against the presumption that matter-antimatter annibilation should necessarily produce large distortions. © 1976 D. Reidel Publishing Company.International Centre for Theoretical Physics, TriesteInstituto de Física Teórica, São PauloInternational Centre for Theoretical PhysicsInstituto de Física TeóricaAldrovandi, R.D'Olival, J. B.S.2022-04-29T08:43:19Z2022-04-29T08:43:19Z1976-10-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article471-477http://dx.doi.org/10.1007/BF00642533Astrophysics and Space Science, v. 44, n. 2, p. 471-477, 1976.0004-640X1572-946Xhttp://hdl.handle.net/11449/23103810.1007/BF006425332-s2.0-34250388397Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAstrophysics and Space Scienceinfo:eu-repo/semantics/openAccess2022-04-29T08:43:19Zoai:repositorio.unesp.br:11449/231038Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T17:15:14.468983Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Lasting recombination and cosmic background radiation spectrum
title Lasting recombination and cosmic background radiation spectrum
spellingShingle Lasting recombination and cosmic background radiation spectrum
Aldrovandi, R.
title_short Lasting recombination and cosmic background radiation spectrum
title_full Lasting recombination and cosmic background radiation spectrum
title_fullStr Lasting recombination and cosmic background radiation spectrum
title_full_unstemmed Lasting recombination and cosmic background radiation spectrum
title_sort Lasting recombination and cosmic background radiation spectrum
author Aldrovandi, R.
author_facet Aldrovandi, R.
D'Olival, J. B.S.
author_role author
author2 D'Olival, J. B.S.
author2_role author
dc.contributor.none.fl_str_mv International Centre for Theoretical Physics
Instituto de Física Teórica
dc.contributor.author.fl_str_mv Aldrovandi, R.
D'Olival, J. B.S.
description The thermal decoupling during recombination and the endurance of this process can significantly deform the black-body background radiation spectrum even in the absence of heating sources. Observational data contradicts a flat standard universe but agrees with a low-density model and with a flat matter-antimatter symmetric universe. Evidence is presented against the presumption that matter-antimatter annibilation should necessarily produce large distortions. © 1976 D. Reidel Publishing Company.
publishDate 1976
dc.date.none.fl_str_mv 1976-10-01
2022-04-29T08:43:19Z
2022-04-29T08:43:19Z
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/10.1007/BF00642533
Astrophysics and Space Science, v. 44, n. 2, p. 471-477, 1976.
0004-640X
1572-946X
http://hdl.handle.net/11449/231038
10.1007/BF00642533
2-s2.0-34250388397
url http://dx.doi.org/10.1007/BF00642533
http://hdl.handle.net/11449/231038
identifier_str_mv Astrophysics and Space Science, v. 44, n. 2, p. 471-477, 1976.
0004-640X
1572-946X
10.1007/BF00642533
2-s2.0-34250388397
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Astrophysics and Space Science
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 471-477
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_ 1808128779822825472

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