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2016

Nonsingular Black Hole

Chamseddine, Ali H., Mukhanov, Viatcheslav

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We consider the Schwarzschild black hole and show how, in a theory with limiting curvature, the physical singularity "inside it" is removed.

The resulting spacetime is geodesically complete.
The internal structure of this nonsingular black hole is analogus to Russian nesting dolls.
Namely, after falling into the black hole of radius $r_{g}$, an observer, instead of being destroyed at the singularity, gets for a short time into the region with limiting curvature.

Nonsingular Black Hole · Around

Built on

V. Mukhanov and R. Brandenberger, A Nonsingular Universe,
1969
Earlier work this paper cites.
S. W. Hawking and R. Penrose, The singularities of gravitational collapse and cosmology,
1970
Earlier work this paper cites.
G. W. Gibbons and S. W. Hawking, Cosmolgical event horizons, thermodynamics and particle creation,
1977
Earlier work this paper cites.

Similar

L. Landau and E. Lifshitz, The Classical Theory of Fields
1980
Cited alongside, same era.
M. Markov, Pis’ma Zh. Eskp. Teor. Fiz. 36
1987
Cited alongside, same era.
V. Frolov, M. Markov and V. Mukhanov, Through a Black Hole into a New Universe?
1989
Cited alongside, same era.
A. H. Chamseddine, V. Mukhanov, Resolving Cosmological Singularities
Cited in the paper.
A. H. Chamseddine, V. Mukhanov, In Preparation
Cited in the paper.

Then

V. Mukhanov, R. Brandenberger, and A. Sornborger, A Cosmological Theory without Singularities,
1993
Later among the works it cites.
A. H. Chamseddine and V. Mukhanov, Mimetic Dark Matter,
2013
Later among the works it cites.
A. H. Chamseddine, V. Mukhanov and A. Vikman, Cosmology with Mimetic Matter,
2014
Later among the works it cites.

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