Future-null singularity due to gravitational collapse
Ashok B. Joshi, Karim Mosani, Pankaj S. Joshi

TL;DR
This paper presents a new gravitational collapse model resulting in a future-null singularity, differing from traditional LTB models, with unique causal structure demonstrated through conformal diagrams.
Contribution
It introduces a novel collapse scenario leading to a future-null singularity, expanding understanding of possible end-states in gravitational collapse.
Findings
Identifies a collapse model with a future-null singularity
Shows the distinct causal structure via conformal diagrams
Differentiates from LTB spacetime end-states
Abstract
In the case of unhindered gravitational collapse of matter cloud governed by the Lemaitre-Tolman-Bondi (LTB) spacetime, the end-state singularity is either locally visible, globally visible or completely hidden. We have a past-null singularity in the first two cases while a future-spacelike singularity in the last case. Here, we show an example of a gravitational collapse model whose end-state is a future-null-singularity (it has a causal property that is unlike the cases involving LTB spacetime). We depict such a distinct causal structure of the singularity by conformal diagrams.
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Geometric Analysis and Curvature Flows
