Sunday, April 7, 2013

I predict a new high energy signal from black holes whose wave length is the geometric mean of the Planck scale Lp with the square root of the area A of the horizon, i.e. (LpA^1/2)^1/2. When applied to our future cosmic de Sitter horizon this is an advanced Wheeler-Feynman signal whose dark energy density is hc/Lp^2A.

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