The Schwarzschild black hole as a point particle

Abstract

The description of a point mass in general relativity (GR) is given in the framework of the field formulation of GR where all the dynamical fields, including the gravitational field, are considered in a fixed background spacetime. With the use of stationary (not static) coordinates non-singular at the horizon, the Schwarzschild solution is presented as a point-like field configuration in a whole background Minkowski space. The requirement of a stable $\eta$-causality stated recently in [J.B.Pitts and W.C.Schieve, Found. Phys., v. 34, 211 (2004)] is used essentially as a criterion for testing configurations.

LATEX, 8 pages, no figures

References in corpus (3)

• Self-Interaction and Gauge Invariance
• Dimensional regularization of the third post-Newtonian dynamics of point particles in harmonic coordinates
• Null Cones and Einstein's Equations in Minkowski Spacetime

Cited by in corpus (3)

• Gauge-Invariant Localization of Infinitely Many Gravitational Energies from All Possible Auxiliary Structures
• A point mass and continuous collapse to a point mass in general relativity
• Black holes of the Vaidya type with flat and (A)dS asymptotics as point particles