Chiral loop quantum supergravity and black hole entropy

preprint2022arXivOpen access

Abstract

Recent work has shown that local supersymmetry on a spacetime boundary in N\mathcal{N}-extended AdS supergravity in chiral variables implies coupling to a boundary OSp(N∣2)C\mathrm{OSp}(\mathcal{N}|2)_{\mathbb{C}} super Chern-Simons theory. We propose a way to calculate the entropy SS for the boundary, in the supersymmetric version of loop quantum gravity, for the minimal case N=1\mathcal{N}=1. We calculate the dimensions of the quantum state spaces of UOSp(1∣2)\mathrm{UOSp}(1|2) super Chern-Simons theory with punctures, and analytically continue, for fixed quantum super area of the surface, to OSp(1∣2)C\mathrm{OSp}(1|2)_{\mathbb{C}}. We find S=aH/4S = a_H/4 for large areas and determine the subleading correction.

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