Bounds on the conical defect parameter from solar system tests

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DC Field	Value	Language
dc.creator	Freire Wilson H. C.	-
dc.creator	Bezerra V. B.	-
dc.creator	Lima J. A. S.	-
dc.date	2000	-
dc.date.accessioned	2013-05-30T00:04:11Z	-
dc.date.available	2013-05-30T00:04:11Z	-
dc.date.issued	2013-05-30	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332000000200022	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2000&volume=30&issue=2&spage=398	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/2969	-
dc.description	We analyse the planetary perihelion precession and the deffection of light in the Schwarzschild field modified by a conical defect. By using observational results from solar system tests of general relativity, we obtain limits on the conical defect parameter <img src="http:/img/fbpe/bjp/v30n2/ses.gif">. For the physical case of a cosmic string the quoted limits are one and three orders weaker than the cosmological bounds.	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	Bounds on the conical defect parameter from solar system tests	-
Appears in Collections:	Physics and Astronomy

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