Energy distribution in a Schwarzschild-like spacetime

dc.creator	Grammenos, T.	en
dc.creator	Radinschi, I.	en
dc.date.accessioned	2015-11-23T10:29:09Z
dc.date.available	2015-11-23T10:29:09Z
dc.date.issued	2007
dc.identifier	10.1007/s10773-006-9259-0
dc.identifier.issn	0020-7748
dc.identifier.uri	http://hdl.handle.net/11615/28191
dc.description.abstract	In this paper, utilizing Moller's energy-momentum complex, we explicitly evaluate the energy and momentum density associated with a metric describing a four-dimensional, Schwarzschild-like, spacetime derived from an effective gravity coupled with a U(1) gauge field in the context of a D3-brane dynamics in the classical regime, i.e., between the asymptotic and the Planck regime.	en
dc.source.uri	<Go to ISI>://WOS:000245430500020
dc.subject	energy-momentum complex	en
dc.subject	effective gravity	en
dc.subject	D-branes	en
dc.subject	CHARGED BLACK-HOLE	en
dc.subject	CYLINDRICAL GRAVITATIONAL-WAVES	en
dc.subject	KERR-NEWMAN	en
dc.subject	SPACETIME	en
dc.subject	KASNER-TYPE UNIVERSE	en
dc.subject	QUASI-LOCAL ENERGY	en
dc.subject	GENERAL-RELATIVITY	en
dc.subject	ANGULAR-MOMENTUM	en
dc.subject	MOLLER PRESCRIPTION	en
dc.subject	CONSERVATION LAWS	en
dc.subject	STATIONARY	en
dc.subject	BEAM	en
dc.subject	Physics, Multidisciplinary	en
dc.title	Energy distribution in a Schwarzschild-like spacetime	en
dc.type	journalArticle	en

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