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arXiv:hep-th/0606146hep-th

(Non)perturbative gravity, nonlocality, and nice slices

Steven B. Giddings

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Abstract

Perturbative dynamics of gravity is investigated for high energy scattering and in black hole backgrounds. In the latter case, a straightforward perturbative analysis fails, in a close parallel to the failure of the former when the impact parameter reaches the Schwarzschild radius. This suggests a flaw in a semiclassical description of physics on spatial slices that intersect both outgoing Hawking radiation and matter that has carried information into a black hole; such slices are instrumental in a general argument for black hole information loss. This indicates a possible role for the proposal that nonperturbative gravitational physics is intrinsically nonlocal.

arXiv comments
21 pages, harvmac. v2: minor wording changes and added references
Journal reference
Phys.Rev.D74:106009,2006
DOI
doi:10.1103/PhysRevD.74.106009
Subjects
hep-thHigh Energy Physics, Theory gr-qcGeneral Relativity and Quantum Cosmology

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    • > more response than I was expecting, thank you. You're welcome. > evaporating black hole must be leaking its information to somewhere The information about the contents of the BH during its formation and growth is in the region of strong gravity. Classically, it's squashed into…

      raattgiftView on HNParent context

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