Scalar field cosmology in three-dimensions

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/3256

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DC Field	Value	Language
dc.creator	Oliveira-Neto G.	-
dc.date	2001	-
dc.date.accessioned	2013-05-30T01:08:18Z	-
dc.date.available	2013-05-30T01:08:18Z	-
dc.date.issued	2013-05-30	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332001000300017	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2001&volume=31&issue=3&spage=456	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/3256	-
dc.description	We study an analytical solution to the Einstein's equations in 2 + 1-dimensions. The space-time is dynamical and has a line symmetry. The matter content is a minimally coupled, massless, scalar field. Depending on the value of certain parameters, this solution represents three distinct space-times. The first one is at space-time. Then, we have a big bang model with a negative curvature scalar and a real scalar field. The last case is a big bang model with event horizons where the curvature scalar vanishes and the scalar field changes from real to purely imaginary.	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	Scalar field cosmology in three-dimensions	-
Appears in Collections:	Physics and Astronomy

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