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Circular cosmic string loop in Brans-Dicke theory

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dc.creator Barros A.
dc.creator Sen A. A.
dc.creator Romero C.
dc.date 2001
dc.date.accessioned 2013-05-30T01:12:49Z
dc.date.available 2013-05-30T01:12:49Z
dc.date.issued 2013-05-30
dc.identifier http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332001000300026
dc.identifier http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2001&volume=31&issue=3&spage=507
dc.identifier.uri http://koha.mediu.edu.my:8181/jspui/handle/123456789/3274
dc.description The gravitational field of a stationary circular cosmic string loop, externally supported against collapse, is investigated in the context of Brans-Dicke theory in the weak field approximation of the field equations. The solution is quasi-conformally related to the corresponding solution in Einstein's General Relativity(GR) and goes over to the corresponding solution in GR when the Brans-Dicke parameter omega becomes infinitely large.
dc.publisher Sociedade Brasileira de Física
dc.source Brazilian Journal of Physics
dc.title Circular cosmic string loop in Brans-Dicke theory


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