Some magnetized bianchi type-III massive string cosmological models in general relativity
Autor(a) principal: | |
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Data de Publicação: | 2008 |
Outros Autores: | |
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=S0103-97332008000500015 |
Resumo: | Some Bianchi type III cosmological models with magnetic field for massive string are investigated. F12 is only the non-vanishing component of electromagnetic field tensor Fij. To get a determinate solution. we have assumed that the expansion (θ) in the model is proportional to the shear (σ). This leads to C = An where A and C are functions of time alone. A particular solution for n = 1 is discussed. The physical implications of the models, are also discussed. |
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Brazilian Journal of Physics |
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Some magnetized bianchi type-III massive string cosmological models in general relativityCosmic massive stringBianchi Type III/MagnetizedSome Bianchi type III cosmological models with magnetic field for massive string are investigated. F12 is only the non-vanishing component of electromagnetic field tensor Fij. To get a determinate solution. we have assumed that the expansion (θ) in the model is proportional to the shear (σ). This leads to C = An where A and C are functions of time alone. A particular solution for n = 1 is discussed. The physical implications of the models, are also discussed.Sociedade Brasileira de Física2008-12-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersiontext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332008000500015Brazilian Journal of Physics v.38 n.4 2008reponame:Brazilian Journal of Physicsinstname:Sociedade Brasileira de Física (SBF)instacron:SBF10.1590/S0103-97332008000500015info:eu-repo/semantics/openAccessUpadhaya,R. D.Dave,Shuchieng2009-01-19T00:00:00Zoai:scielo:S0103-97332008000500015Revistahttp://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:2009-01-19T00:00Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF)false |
dc.title.none.fl_str_mv |
Some magnetized bianchi type-III massive string cosmological models in general relativity |
title |
Some magnetized bianchi type-III massive string cosmological models in general relativity |
spellingShingle |
Some magnetized bianchi type-III massive string cosmological models in general relativity Upadhaya,R. D. Cosmic massive string Bianchi Type III/Magnetized |
title_short |
Some magnetized bianchi type-III massive string cosmological models in general relativity |
title_full |
Some magnetized bianchi type-III massive string cosmological models in general relativity |
title_fullStr |
Some magnetized bianchi type-III massive string cosmological models in general relativity |
title_full_unstemmed |
Some magnetized bianchi type-III massive string cosmological models in general relativity |
title_sort |
Some magnetized bianchi type-III massive string cosmological models in general relativity |
author |
Upadhaya,R. D. |
author_facet |
Upadhaya,R. D. Dave,Shuchi |
author_role |
author |
author2 |
Dave,Shuchi |
author2_role |
author |
dc.contributor.author.fl_str_mv |
Upadhaya,R. D. Dave,Shuchi |
dc.subject.por.fl_str_mv |
Cosmic massive string Bianchi Type III/Magnetized |
topic |
Cosmic massive string Bianchi Type III/Magnetized |
description |
Some Bianchi type III cosmological models with magnetic field for massive string are investigated. F12 is only the non-vanishing component of electromagnetic field tensor Fij. To get a determinate solution. we have assumed that the expansion (θ) in the model is proportional to the shear (σ). This leads to C = An where A and C are functions of time alone. A particular solution for n = 1 is discussed. The physical implications of the models, are also discussed. |
publishDate |
2008 |
dc.date.none.fl_str_mv |
2008-12-01 |
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=S0103-97332008000500015 |
url |
http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332008000500015 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
10.1590/S0103-97332008000500015 |
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.38 n.4 2008 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_ |
1754734864768172032 |