The principled-parameterized approach to gravitational collapse
H\'elo\"ise Delaporte, Astrid Eichhorn

TL;DR
This paper applies a principle-based method to modify black-hole spacetimes for gravitational collapse, aiming to incorporate new physics beyond General Relativity while ensuring regularity and analyzing geodesic behavior.
Contribution
It extends the principled-parameterized approach to time-dependent collapsing spacetimes, demonstrating regularization and geodesic completeness in dynamic black-hole models.
Findings
Vaidya spacetime becomes regular with modifications
Null geodesics can be future complete due to the modifications
Violations of null energy condition occur inside the apparent horizon
Abstract
New physics beyond General Relativity impacts black-hole spacetimes. The effects of new physics can be investigated in a largely theory-agnostic way by following the principled-parameterized approach. In this approach, a classical black-hole metric is upgraded by following a set of principles, such as regularity, i.e., the absence of curvature singularities. We expect these principles to hold in many theories beyond General Relativity. In the present paper, we implement this approach for time-dependent spacetimes describing gravitational collapse. We find that the Vaidya spacetime becomes regular through the same modification of the spacetime metric as stationary black-hole spacetimes [1-3]. We investigate null geodesics and find indications that the modification is even sufficient to render null geodesics future complete. Finally, we find that the modification of the spacetime…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory
