The Thermodynamics of the Gravity from Entropy Theory
Ginestra Bianconi

TL;DR
This paper explores a thermodynamic interpretation of gravity derived from entropy principles, proposing a modified theory that reduces to Einstein's gravity under certain conditions and exhibits non-decreasing entropy in cosmological models.
Contribution
It introduces the Gravity from Entropy (GfE) action based on geometric quantum relative entropy, linking gravity to thermodynamics and providing a new framework for cosmology.
Findings
GfE universes admit a thermodynamic description with k-temperatures and k-pressures.
In low energy regimes, GfE solutions approximate Friedmann cosmologies.
Total entropy of GfE universes is non-decreasing over time.
Abstract
The Gravity from Entropy (GfE) action posits that gravity that is fundamentally given by the information encoded in the interplay between matter and geometry. The GfE Lagrangian is given by the Geometric Quantum Relative Entropy (GQRE) between the physical metric and the metric induced by matter and curvature, leading to modified gravitational field equations with an emergent dynamical effective dark energy term, which reduce to Einstein's equations in the low energy, small curvature limit. Adopting a thermodynamic viewpoint, we identify the GfE energy density with this emergent effective dark energy term. For homogeneous and isotropic FRW spacetimes, we show that GfE universes admit a thermal description: locally, they are characterized by -temperatures and -pressures satisfying a first law of GfE thermodynamics. In the low energy, small curvature regime with perfect-fluid matter…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
