Particle creation in the marginally bound, self-similar collapse of inhomogeneous dust
References (18)
Comm. Math. Phys.
(1975)Global Aspects in Gravitation and Cosmology
(1993)- et al.
Phys. Rev.
(1993) Mon. Not. Astron. Soc.
(1947)- et al.
Commun. Math. Phys.
(1973)et al.Commun. Math. Phys.
(1974)et al.Phys. Rev. D
(1979)Commun. Math. Phys.
(1984)Class. Quant. Grav.
(1986)et al.Phys. Rev. D
(1988)et al.Phys. Lett. A
(1989)Class. Quant. Grav.
(1991)et al.Gen. Rel. Grav.
(1991)et al.Prog. Theor. Phys.
(1991)et al.Phys. Rev D
(1993)et al.Comm. Math. Phys.
(1994)et al.Class. Quant. Grav.
(1996)et al.Class. Quant. Grav.
(1997) - et al.
Class. Quant. Grav.
(1996) - et al.
Phys. Rev. D
(1982)Prog. Theor. Phys.
(1984)Class. Quant. Grav.
(1986)Can. J. Phys.
(1986)et al.Phys. Rev. D
(1987)Phys. Rev. Lett.
(1992) - et al.
Phys. Rev. D
(1990)
Cited by (43)
Quantum gravitational dust collapse does not result in a black hole
2015, Nuclear Physics BCitation Excerpt :This leaves just the first option, that the Hawking radiation is pure. In 1993, Susskind et al. [7], building on the work of 't Hooft [8] and Preskill [9], proposed that the unitarity of the Hawking radiation could be preserved if information is both emitted at the horizon and passes through it, so an observer outside would see it in the Hawking radiation and an observer who falls into the black hole would see it inside but no single observer would be able to confirm both pictures. Although there is no precise mechanism by which it can be said to occur, thought experiments that appear to support this picture of “Black Hole Complementarity” rely on three fundamental assumptions, viz., (a) the unitarity of the Hawking radiation, (b) the validity of effective field theory outside a “stretched” horizon and (c) the equivalence principle.
Observational testability of a Kerr bound in the x-ray spectrum of black hole candidates
2010, Classical and Quantum GravityEffects of Lovelock terms on the final fate of gravitational collapse: Analysis in dimensionally continued gravity
2006, Classical and Quantum GravityPhysical aspects of a naked singularity explosion: How does a naked singularity explode?
2001, Classical and Quantum GravityParticle creation in gravitational collapse to a horizonless compact object
2019, Physical Review D