| dc.contributor.author | Kinyanjui, Carringtone | |
| dc.contributor.author | Wamalwa, Dismas S | |
| dc.date.accessioned | 2021-12-15T07:01:57Z | |
| dc.date.available | 2021-12-15T07:01:57Z | |
| dc.date.issued | 2017 | |
| dc.identifier.uri | http://repository.must.ac.ke/handle/123456789/567 | |
| dc.description.abstract | A reformulation of the Schwarzschild solution of the linearized Einstein field equations in post-Riemannian Finsler spacetime is derived. The solution is constructed in three stages: the exterior solution, the event-horizon solution and the interior solution. It is shown that the exterior solution is asymptotically similar to Newtonian gravity at large distances implying that Newtonian gravity is a low energy approximation of the solution. Application of Eddington-Finklestein coordinates is shown to reproduce the results obtained from standard general relativity at the event horizon. Further application of Kruskal-Szekeres coordinates reveals that the interior solution contains maximally extensible geodesics | en_US |
| dc.language.iso | en | en_US |
| dc.subject | Einstein field equations, | en_US |
| dc.subject | Schwarzschild metric, | en_US |
| dc.subject | Black holes, Finsler spaces | en_US |
| dc.title | Schwarzschild solution of the modified Einstein field equations | en_US |
| dc.type | Article | en_US |
