Systolic Aspects of Black Hole Entropy

Systolic Aspects of Black Hole Entropy

Blog Article

We attempt to provide a mesoscopic treatment of the origin of black hole entropy in (3 + 1)-dimensional spacetimes.We ascribe this entropy to the non-trivial topology of the space-like sections Σ wahl kmx of the horizon.This is not forbidden by topological censorship, since all the known energy inequalities needed to prove the spherical topology of Σ are violated in quantum theory.We choose the systoles of Σ to encode its complexity, which gives rise to the black hole entropy.We present hand-waving reasons why the entropy of the black hole can be considered as a function of the volume entropy of Σ.

We focus on the limiting case of biffy clyro vinyl offers Σ having a large genus.