Abstract
Abstract
We discuss back-reaction in the semiclassical treatment of quantum fields near a black hole. When the state deviates significantly from Hartle-Hawking, simple energetic considerations of back-reaction give rise to a characteristic radial distance scale ∼ $$ {\left({r}_s^2{G}_N\right)}^{1/D} $$
r
s
2
G
N
1
/
D
, below which some breakdown of effective field theory may occur.
Publisher
Springer Science and Business Media LLC
Cited by
1 articles.
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