(Non)perturbative gravity, nonlocality, and nice slices

Jun, 2006
22 pages
Published in:
  • Phys.Rev.D 74 (2006) 106009
e-Print:

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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.
  • 04.60.-m
  • 11.25.Sq
  • 04.70.Dy
  • gravitation
  • background field
  • fluctuation
  • radiation: Hawking
  • approximation: semiclassical
  • field theory: nonlocal
  • black hole