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 |