dc.creator | Radinschi, I. | en |
dc.creator | Grammenos, T. | en |
dc.creator | Spanou, A. | en |
dc.date.accessioned | 2015-11-23T10:46:17Z | |
dc.date.available | 2015-11-23T10:46:17Z | |
dc.date.issued | 2013 | |
dc.identifier | 10.1007/s10773-012-1384-3 | |
dc.identifier.issn | 0020-7748 | |
dc.identifier.uri | http://hdl.handle.net/11615/32570 | |
dc.description.abstract | In general relativity one of the most fundamental issues consists in defining a generally acceptable definition for the energy-momentum density. As a consequence, many coordinate-dependent definitions have been presented, whereby some of them utilize appropriate energy-momentum complexes. We investigate the energy-momentum distribution for a metric exterior to a spherically symmetric black hole in the brane world by applying the Landau-Lifshitz and Weinberg prescriptions. In both the aforesaid prescriptions, the energy thus obtained depends on the radial coordinate, the mass of the black hole and a parameter lambda (0), while all the momenta are found to be zero. It is shown that for a special value of the parameter lambda (0), the Schwarzschild space-time geometry is recovered. Some particular and limiting cases are also discussed. | en |
dc.source.uri | <Go to ISI>://WOS:000314533100009 | |
dc.subject | Energy-momentum complexes | en |
dc.subject | Brane world black holes | en |
dc.subject | GENERAL-RELATIVITY | en |
dc.subject | ANGULAR-MOMENTUM | en |
dc.subject | TELEPARALLEL GRAVITY | en |
dc.subject | STATIONARY | en |
dc.subject | BEAM | en |
dc.subject | MODELS | en |
dc.subject | SYSTEM | en |
dc.subject | LIGHT | en |
dc.subject | MASS | en |
dc.subject | Physics, Multidisciplinary | en |
dc.title | Energy-Momentum Localization for a Space-Time Geometry Exterior to a Black Hole in the Brane World | en |
dc.type | journalArticle | en |