Angular momentum conservation for uniformly expanding flows
| dc.creator | Hayward, Sean A. | |
| dc.date | 2006-11-04 | |
| dc.date.accessioned | 2026-07-07T10:21:59Z | |
| dc.date.available | 2026-07-07T10:21:59Z | |
| dc.description | Angular momentum has recently been defined as a surface integral involving an axial vector and a twist 1-form, which measures the twisting around of space-time due to a rotating mass. The axial vector is chosen to be a transverse, divergence-free, coordinate vector, which is compatible with any initial choice of axis and integral curves. Then a conservation equation expresses rate of change of angular momentum along a uniformly expanding flow as a surface integral of angular momentum densities, with the same form as the standard equation for an axial Killing vector, apart from the inclusion of an effective energy tensor for gravitational radiation. | |
| dc.description | 5 revtex4 pages, 3 eps figures | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0611027 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0611027 | |
| dc.identifier | Class.Quant.Grav.24:923-930,2007 | |
| dc.identifier | doi:10.1088/0264-9381/24/4/012 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/175361 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Angular momentum conservation for uniformly expanding flows | |
| dc.type | text |