SCHWARZSCHILD SOLUTION OF THE MODIFIED EINSTEIN FIELD EQUATIONS

Journal Title: JOURNAL OF ADVANCES IN PHYSICS - Year 2017, Vol 13, Issue 5

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.

Authors and Affiliations

D. S. Wamalwa, Carringtone Kinyanjui

Keywords

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  • EP ID EP653375
  • DOI 10.24297/jap.v13i5.6132
  • Views 73
  • Downloads 0

How To Cite

D. S. Wamalwa, Carringtone Kinyanjui (2017). SCHWARZSCHILD SOLUTION OF THE MODIFIED EINSTEIN FIELD EQUATIONS. JOURNAL OF ADVANCES IN PHYSICS, 13(5), 4895-4900. https://europub.co.uk/articles/-A-653375