Spacetime Dynamics and Local Entropy Balance on Causal Horizons
Abstract
We propose that spacetime dynamics can be organized by a Planck-scale bookkeeping rule, written using a modular-parameter normalization of size , that balances the geometric entropy increment against a reversible modular-energy flow and an irreversible Landauer--Bennett cost , where is the (dimensionless) modular Hamiltonian of the chosen region defined relative to a fixed reference state , and counts logically irreversible one-bit record updates (e.g. coarse-grained overwrites or registrations) on that screen. This ``information--geometry ledger'' is consistent with the Bekenstein--Hawking area law and, when enforced on small causal screens under the standard entanglement-equilibrium assumptions, recovers the full nonlinear Einstein equation. In FLRW cosmology, the same bookkeeping motivates a two-component vacuum sector when a constant inefficiency parameter is assumed.
Keywords
Cite
@article{arxiv.2512.17961,
title = {Spacetime Dynamics and Local Entropy Balance on Causal Horizons},
author = {Daegene Song},
journal= {arXiv preprint arXiv:2512.17961},
year = {2026}
}
Comments
5 pages