pith. machine review for the scientific record. sign in

arxiv: gr-qc/9603025 · v3 · submitted 1996-03-15 · 🌀 gr-qc

Recognition: unknown

Counting surface states in the loop quantum gravity

Authors on Pith no claims yet
classification 🌀 gr-qc
keywords quantumstatessurfacealphaareaclassicalensembleentropy
0
0 comments X
read the original abstract

We adopt the point of view that (Riemannian) classical and (loop-based) quantum descriptions of geometry are macro- and micro-descriptions in the usual statistical mechanical sense. This gives rise to the notion of geometrical entropy, which is defined as the logarithm of the number of different quantum states which correspond to one and the same classical geometry configuration (macro-state). We apply this idea to gravitational degrees of freedom induced on an arbitrarily chosen in space 2-dimensional surface. Considering an `ensemble' of particularly simple quantum states, we show that the geometrical entropy $S(A)$ corresponding to a macro-state specified by a total area $A$ of the surface is proportional to the area $S(A)=\alpha A$, with $\alpha$ being approximately equal to $1/16\pi l_p^2$. The result holds both for case of open and closed surfaces. We discuss briefly physical motivations for our choice of the ensemble of quantum states.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Hawking radiation from black holes in 2+1 dimensions

    gr-qc 2026-04 unverdicted novelty 6.0

    Black hole horizons in 2+1D are composed of quantized length quanta 8π ℓ_P n, producing entropy near the Bekenstein-Hawking value and a local Hawking spectrum via a length ensemble.

  2. Hawking radiation from black holes in 2+1 dimensions

    gr-qc 2026-04 unverdicted novelty 3.0

    In 2+1 dimensions, black hole horizons are quantized into lengths 8π ℓ_P n, from which a length ensemble directly yields the Hawking blackbody spectrum with Tolman-modified temperature.