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2015

Quantum black hole without singularity

Kiefer, Claus

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We discuss the quantization of a spherical dust shell in a rigorous manner.

Classically, the shell can collapse to form a black hole with a singularity.
In the quantum theory, we construct a well-defined self-adjoint extension for the Hamilton operator.
As a result, the evolution is unitary and the singularity is avoided.

Quantum black hole without singularity · Around

Built on

B. S. DeWitt, Phys. Rev
1967
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C. Kiefer and H. D. Zeh, Phys. Rev. D
Original
1995
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B. K. Berger, D. M. Chitre, V. E. Moncrief, and Y. Nutku, Phys. Rev. D
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P. Hájíček and J. Kijowski, Phys. Rev. D
2000
Earlier work this paper cites.
P. Hájíček and C. Kiefer, Nucl. Phys. B
2001
Earlier work this paper cites.

Similar

P. Hájíček, Nucl. Phys. B
2001
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P. Hájíček and C. Kiefer, Int. J. Mod. Phys. D
2001
Cited alongside, same era.
P. Hájíček, in: Quantum Gravity: From Theory to Experimental Search
2003
Cited alongside, same era.
M. Ambrus and P. Hájíček, Phys. Rev. D
2005
Cited alongside, same era.
C. Kiefer, J. Marto, and P. V. Moniz, Ann. Phys. (Berlin)
2009
Cited alongside, same era.

Then

M. Bouhmadi-López, C. Kiefer, B. Sandhöfer, and P. V. Moniz, Phys. Rev. D
2009
Later among the works it cites.
C. Kiefer, Quantum Gravity
2012
Later among the works it cites.
H. M. Haggard and C. Rovelli, Phys. Rev. D
2015
Closest in time.
A. Barrau, C. Rovelli, and F. Vidotto, Phys. Rev. D
Original
2015
Closest in time.

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