# Physical black holes in semiclassical gravity

@article{Murk2021PhysicalBH, title={Physical black holes in semiclassical gravity}, author={Sebastian Murk and Daniel R. Terno}, journal={The Sixteenth Marcel Grossmann Meeting}, year={2021} }

We derive and critically examine the consequences that follow from the formation of a regular black or white hole horizon in ﬁnite time of a distant observer. In spherical symmetry, only two distinct classes of solutions to the semiclassical Einstein equations are self-consistent. Both are required to describe the formation of physical black holes and violate the null energy condition in the vicinity of the outer apparent horizon. The near-horizon geometry diﬀers considerably from that of…

## One Citation

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