28 citations · 214 across the 21 of their papers we have counts for
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Black holes and their horizons in semiclassical and modified theories of gravity
Robert B. Mann, Sebastian Murk, Daniel R. Terno
For distant observers black holes are trapped spacetime domains bounded by apparent horizons. We review properties of the near-horizon geometry emphasizing the consequences of two…
Constraining modified gravity theories with physical black holes
Sebastian Murk
We review the constraints modified theories of gravity must satisfy to be compatible with the spherically symmetric black hole solutions of semiclassical gravity that describe the…
Physical black holes in fourth-order gravity
Sebastian Murk
The existence of black holes is a central prediction of general relativity and thus serves as a basic consistency test for modified theories of gravity. In spherical symmetry, only…
Physical black holes in semiclassical gravity
Sebastian Murk, Daniel R. Terno
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 symmetr…
Semiclassical black holes and horizon singularities
Pravin K. Dahal, Sebastian Murk, Daniel R. Terno
In spherical symmetry, solutions of the semiclassical Einstein equations belong to one of two possible classes. Both classes contain solutions that -- depending on the dynamic beha…
Paradoxes before the paradox: surface gravity and the information loss problem
Robert B. Mann, Sebastian Murk, Daniel R. Terno
The information loss paradox is widely regarded as one of the biggest open problems in theoretical physics. Several classical and quantum features must be present to enable its for…