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Gravitational Collapse for the K-essence Emergent Vaidya Spacetime

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abstract

In this paper, we study the gravitational collapse in the {\bf k-}essence emergent gravity using a generalized Vaidya-type metric as a background. We also analyze the cosmic censorship hypothesis for this system. We show that the emergent gravity metric resembles closely to the new type of the generalized Vaidya metrics for null fluid collapse with the {\bf k-}essence emergent mass function, where we consider the {\bf k-}essence scalar field being a function solely of the advanced or the retarded time. This new type of {\bf k-}essence emergent Vaidya metric has satisfied the required energy conditions. The existence of the locally naked central singularity, the strength and the strongness of the singularities for the {\bf k-}essence emergent Vaidya metric are the interesting outcomes of the present work.

fields

gr-qc 1

years

2025 1

verdicts

CONDITIONAL 1

representative citing papers

K-essence sources of Kerr-Schild spacetimes

gr-qc · 2025-04-19 · conditional · novelty 6.0

K-essence Lagrangians that can source Kerr-Schild spacetimes must be at most quadratic in the kinetic term, and linear when the congruence is autoparallel or when linearized solutions are also exact.

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  • K-essence sources of Kerr-Schild spacetimes gr-qc · 2025-04-19 · conditional · none · ref 29 · internal anchor

    K-essence Lagrangians that can source Kerr-Schild spacetimes must be at most quadratic in the kinetic term, and linear when the congruence is autoparallel or when linearized solutions are also exact.