English

An Extension of Schwarzschild Space to r=0

General Relativity and Quantum Cosmology 2009-10-31 v2

Abstract

A more rigorous treatment of the Schwarzschild metric by making use of the energy-momentum tensor of a single point particle as source term shows that g00={12GMc2r8G2M2c4r2(θ(r)1)}exp[2(θ(r)1)]g_{00}=-\{1-\frac{2GM}{c^2r}-\frac{8G^2 M^2}{c^4 r^2}(\theta (r)-1)\}\exp [2(\theta (r)-1)] grr={12GMc2r8G2M2c4r2(θ(r)1)}1g_{rr}=\{1-\frac{2GM}{c^2r}-\frac{8G^2 M^2}{c^4 r^2}(\theta (r)-1)\}^{-1} The existence of a discontinuity at r=0 leads to an infinite repulsive force that will change the ultimate fate of a free fall test particle to a bouncing state.

Keywords

Cite

@article{arxiv.gr-qc/9912022,
  title  = {An Extension of Schwarzschild Space to r=0},
  author = {Amir H. Abbassi},
  journal= {arXiv preprint arXiv:gr-qc/9912022},
  year   = {2009}
}

Comments

16 pages, no figure, some errors are corrected, two sections on tidal forces and Riemann scalar invariant are added. To appear in Physica Scripta