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 |