Pulsar binary systems in a nonsymmetric theory of gravitation II. Dipole radiation
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Data de Publicação: | 2010 |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Brazilian Journal of Physics |
Texto Completo: | http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332010000400009 |
Resumo: | This paper deals with the emission of gravitational radiation in the context of a previously studied metric nonsymmetric theory of gravitation. The part coming from the symmetric part of the metric coincides with the mass quadrupole moment result of general relativity. The one associated to the antisymmetric part of the metric involves the dipole moment of the fermionic charge of the system. The results are applied to binary star systems and the decrease of the period of the elliptical motion is calculated. |
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Brazilian Journal of Physics |
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|
spelling |
Pulsar binary systems in a nonsymmetric theory of gravitation II. Dipole radiationdipole radiationnonsymmetricThis paper deals with the emission of gravitational radiation in the context of a previously studied metric nonsymmetric theory of gravitation. The part coming from the symmetric part of the metric coincides with the mass quadrupole moment result of general relativity. The one associated to the antisymmetric part of the metric involves the dipole moment of the fermionic charge of the system. The results are applied to binary star systems and the decrease of the period of the elliptical motion is calculated.Sociedade Brasileira de Física2010-12-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersiontext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332010000400009Brazilian Journal of Physics v.40 n.4 2010reponame:Brazilian Journal of Physicsinstname:Sociedade Brasileira de Física (SBF)instacron:SBF10.1590/S0103-97332010000400009info:eu-repo/semantics/openAccessRagusa,S.eng2011-01-03T00:00:00Zoai:scielo:S0103-97332010000400009Revistahttp://www.sbfisica.org.br/v1/home/index.php/pt/ONGhttps://old.scielo.br/oai/scielo-oai.phpsbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br1678-44480103-9733opendoar:2011-01-03T00:00Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF)false |
dc.title.none.fl_str_mv |
Pulsar binary systems in a nonsymmetric theory of gravitation II. Dipole radiation |
title |
Pulsar binary systems in a nonsymmetric theory of gravitation II. Dipole radiation |
spellingShingle |
Pulsar binary systems in a nonsymmetric theory of gravitation II. Dipole radiation Ragusa,S. dipole radiation nonsymmetric |
title_short |
Pulsar binary systems in a nonsymmetric theory of gravitation II. Dipole radiation |
title_full |
Pulsar binary systems in a nonsymmetric theory of gravitation II. Dipole radiation |
title_fullStr |
Pulsar binary systems in a nonsymmetric theory of gravitation II. Dipole radiation |
title_full_unstemmed |
Pulsar binary systems in a nonsymmetric theory of gravitation II. Dipole radiation |
title_sort |
Pulsar binary systems in a nonsymmetric theory of gravitation II. Dipole radiation |
author |
Ragusa,S. |
author_facet |
Ragusa,S. |
author_role |
author |
dc.contributor.author.fl_str_mv |
Ragusa,S. |
dc.subject.por.fl_str_mv |
dipole radiation nonsymmetric |
topic |
dipole radiation nonsymmetric |
description |
This paper deals with the emission of gravitational radiation in the context of a previously studied metric nonsymmetric theory of gravitation. The part coming from the symmetric part of the metric coincides with the mass quadrupole moment result of general relativity. The one associated to the antisymmetric part of the metric involves the dipole moment of the fermionic charge of the system. The results are applied to binary star systems and the decrease of the period of the elliptical motion is calculated. |
publishDate |
2010 |
dc.date.none.fl_str_mv |
2010-12-01 |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332010000400009 |
url |
http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332010000400009 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
10.1590/S0103-97332010000400009 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
text/html |
dc.publisher.none.fl_str_mv |
Sociedade Brasileira de Física |
publisher.none.fl_str_mv |
Sociedade Brasileira de Física |
dc.source.none.fl_str_mv |
Brazilian Journal of Physics v.40 n.4 2010 reponame:Brazilian Journal of Physics instname:Sociedade Brasileira de Física (SBF) instacron:SBF |
instname_str |
Sociedade Brasileira de Física (SBF) |
instacron_str |
SBF |
institution |
SBF |
reponame_str |
Brazilian Journal of Physics |
collection |
Brazilian Journal of Physics |
repository.name.fl_str_mv |
Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF) |
repository.mail.fl_str_mv |
sbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br |
_version_ |
1754734865445552128 |