An improved estimate of black hole entropy in the quantum geometry approach

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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5 pages, LaTeX; references and remarks added

Scientific paper

10.1016/j.physletb.2005.05.003

A proper counting of states for black holes in the quantum geometry approach
shows that the dominant configuration for spins are distributions that include
spins exceeding one-half at the punctures. This raises the value of the Immirzi
parameter and the black hole entropy. However, the coefficient of the
logarithmic correction remains -1/2 as before.

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