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arXiv:hep-th/0409131hep-th

Black Holes from Colliding Wavepackets

Steven B. Giddings, Vyacheslav S. Rychkov

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Abstract

Arguments for black hole formation in collisions of high-energy particles have rested on the emergence of a closed trapped surface in the classical geometry of two colliding Aichelburg-Sexl solutions. Recent analysis has, however, shown that curvatures and quantum fluctuations are large on this apparent horizon, potentially invalidating a semiclassical analysis. We show that this problem is an artifact of the unphysical classical point-particle limit: for a particle described by a quantum wavepacket, or for a continuous matter distribution, trapped surfaces indeed form in a controlled regime.

arXiv comments
6 pages
Journal reference
Phys.Rev. D70 (2004) 104026
DOI
doi:10.1103/PhysRevD.70.104026
Subjects
hep-thHigh Energy Physics, Theory gr-qcGeneral Relativity and Quantum Cosmology hep-phHigh Energy Physics, Phenomenology

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  1. The Unraveling of Space-Time 1 comment
    • The idea of making the black hole membrane paradigm generally covariant and everywhere locally Lorentz invariant gives me a migraine. Dropping charges onto a superthin surface (and keeping it cold, we have to consider arbitrarily large SMBHs too) or having the superthin surface…

      raattgiftView on HNParent context

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