Gravitational collapses to bodies of a finite volume

Abstract

We prove with an exact relativistic computation that the spherosymmetric gravitational collapses with a time-dependent pressure end in bodies with a small, but finite volume. Against a diffuse, wrong conviction.

8 pages, LaTeX, to be published on Spacetime & Substance

References in corpus (2)

• No GW is emitted by B PSR1913+16
• No motions of bodies produce GW's

Cited by in corpus (4)

• On spherically symmetric structures in GR
• Gravitational collapses and Hilbertian repulsion
• Highest-Energy Cosmic Rays and Hilbertian Repulsive Effect
• On some relativistic singular surfaces