
TL;DR
This paper proposes that all types of spacetime horizons share microscopic properties, which could serve as foundational postulates for developing a microscopic theory of gravity.
Contribution
It introduces the idea that diverse horizons have common microscopic features, providing a new basis for formulating a microscopic theory of gravity.
Findings
All horizons share certain microscopic properties.
These properties can serve as postulates for gravity theories.
Potential unification of horizon physics across different spacetime geometries.
Abstract
We suggest that all horizons of spacetime, no matter whether they are black hole, Rindler or de Sitter horizons, have certain microscopic properties in common. We propose that these propertues may be used as the starting points, or postulates, of a microscopic theory of gravity.
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Taxonomy
TopicsPoint processes and geometric inequalities
