Outer Trapped Surfaces in Vaidya Spacetimes
classification
🌀 gr-qc
keywords
outerspacetimessurfacestrappedcontainingeventhorizonregion
read the original abstract
It is proven that in Vaidya spacetimes of bounded total mass, the outer boundary, in spacetime, of the region containing outer trapped surfaces, is the event horizon. Further, it is shown that the region containing trapped surfaces in these spacetimes does not always extend to the event horizon.
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Cited by 1 Pith paper
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Regular Vaidya solutions of effective gravitational theories
Regular Vaidya solutions exist in effective gravitational theories that dynamically describe radiation-driven formation of regular black holes or mimickers without curvature singularities.
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