Pseudoenergy, Superenergy, and Energy Radiation via Gravitational Waves in General Relativity
| dc.creator | Pokrovsky, Yury E. | |
| dc.date | 2003-05-27 | |
| dc.date.accessioned | 2026-07-07T12:21:18Z | |
| dc.date.available | 2026-07-07T12:21:18Z | |
| dc.description | For slowly spinning matter the rate of energy loss via radiation of gravitational waves is estimated in General Relativity (GR) within a generally covariant superenergy approach. This estimation differs from Einstein's Quadrupole Formula (EQF) by a suppression factor ($Π\ll1$). For a symmetric two-body-like distribution of scalar matter $Π$ is estimated to be $\ll(v/c)^2(r/R)^2$, where $v$ is orbital velocity of the bodies, $c$ - velocity of light, $r$ - radius of each body, and $R$ -- the inter-body distance. This contradiction with EQF is briefly discussed. | |
| dc.description | 4 pages, 1 figures | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0305100 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0305100 | |
| dc.identifier | Grav.Cosmol.9:95-98,2003 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/213320 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Pseudoenergy, Superenergy, and Energy Radiation via Gravitational Waves in General Relativity | |
| dc.type | text |