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Collapsing scenario for the k-essence emergent generalised Vaidya spacetime in the context of massive gravity's rainbow

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arxiv 2208.05778 v1 pith:BBY3Y3W4 submitted 2022-08-10 gr-qc hep-th

Collapsing scenario for the k-essence emergent generalised Vaidya spacetime in the context of massive gravity's rainbow

classification gr-qc hep-th
keywords gravityk-essencemassiverainbowvaidyaemergentmetricspacetime
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In this paper, we study the collapsing scenario for the k-essence emergent Vaidya spacetime in the context of massive gravity's rainbow. For this study, we consider that the background metric is Vaidya spacetime in massive gravity's rainbow. We show that the k-essence emergent gravity metric resembles closely to the new type of generalized Vaidya massive gravity metric with the rainbow deformations for null fluid collapse where we consider the k-essence scalar field as a function solely of the advanced or the retarded time. The k-essence emergent Vaidya massive gravity rainbow mass function is also different. This new type k-essence emergent Vaidya massive gravity rainbow 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 rainbow deformations of the k-essence emergent Vaidya massive gravity metric are the interesting outcomes of the present work.

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  1. Shadow of the generalized Vaidya black hole

    gr-qc 2026-07 conditional novelty 5.0

    For self-similar Husain black holes, the barotropic index α controls the shadow: α<1/2 enlarges it, α>1/2 shrinks it, with a quasistatic influx criterion for the time-dependent case.