Energy and momentum distributions of the magnetic solution to (2+1) Einstein-Maxwell gravity

dc.creator	Grammenos, T.	en
dc.date.accessioned	2015-11-23T10:29:09Z
dc.date.available	2015-11-23T10:29:09Z
dc.date.issued	2005
dc.identifier	10.1142/s0217732305016956
dc.identifier.issn	0217-7323
dc.identifier.uri	http://hdl.handle.net/11615/28189
dc.description.abstract	We use Moller's energy-momentum complex in order to explicitly evaluate the energy and momentum density distributions associated with the three-dimensional magnetic solution to the Einstein-Maxwell equations. The magnetic spacetime under consideration is a one-parametric solution describing the distribution of a radial magnetic field in a three-dimensional AdS background, and representing the superposition of the magnetic field with a 2+1 Einstein static gravitational field.	en
dc.source.uri	<Go to ISI>://WOS:000231204900004
dc.subject	energy-momentum complex	en
dc.subject	Einstein-Maxwell gravity	en
dc.subject	AdS(3) spacetime	en
dc.subject	QUASI-LOCAL ENERGY	en
dc.subject	CYLINDRICAL GRAVITATIONAL-WAVES	en
dc.subject	SCHWARZSCHILD	en
dc.subject	BLACK-HOLE	en
dc.subject	KERR-NEWMAN SPACETIME	en
dc.subject	GENERAL-RELATIVITY	en
dc.subject	ANGULAR-MOMENTUM	en
dc.subject	ADS/CFT CORRESPONDENCE	en
dc.subject	MOLLER PRESCRIPTION	en
dc.subject	STRESS TENSOR	en
dc.subject	MASS	en
dc.subject	Physics, Nuclear	en
dc.subject	Physics, Particles & Fields	en
dc.subject	Physics, Mathematical	en
dc.title	Energy and momentum distributions of the magnetic solution to (2+1) Einstein-Maxwell gravity	en
dc.type	journalArticle	en

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