Gravitational collapses to bodies of a finite volume
Tiziana Marsico, Angelo Loinger

TL;DR
This paper demonstrates through exact relativistic calculations that spherically symmetric gravitational collapses with time-dependent pressure result in finite-volume bodies, challenging the common misconception of diffuse outcomes.
Contribution
It provides a rigorous relativistic proof that gravitational collapses can produce finite-sized bodies, countering previous diffuse assumptions.
Findings
Collapse results in finite-volume bodies
Relativistic computation confirms finite size
Challenges diffuse collapse assumptions
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.
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Geophysics and Gravity Measurements
