The paper proposes that the black hole singularity, modeled as a random network of elementary degrees of freedom, carries entropy proportional to M^2, matching the scaling of Bekenstein-Hawking entropy.
(Quantum) Space-Time as a Statistical Geometry of Fuzzy Lumps and the Connection with Random Metric Spaces
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
We develop a kind of pregeometry consisting of a web of overlapping fuzzy lumps which interact with each other. The individual lumps are understood as certain closely entangled subgraphs (cliques) in a dynamically evolving network which, in a certain approximation, can be visualized as a time-dependent random graph. This strand of ideas is merged with another one, deriving from ideas, developed some time ago by Menger et al, that is, the concept of probabilistic- or random metric spaces, representing a natural extension of the metrical continuum into a more microscopic regime. It is our general goal to find a better adapted geometric environment for the description of microphysics. In this sense one may it also view as a dynamical randomisation of the causal-set framework developed by e.g. Sorkin et al. In doing this we incorporate, as a perhaps new aspect, various concepts from fuzzy set theory.
fields
gr-qc 1years
2024 1verdicts
REJECT 1representative citing papers
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The Black Hole Singularity as a Thermodynamic System being the Seat of BH Entropy
The paper proposes that the black hole singularity, modeled as a random network of elementary degrees of freedom, carries entropy proportional to M^2, matching the scaling of Bekenstein-Hawking entropy.