Towards a causal effective thermodynamics of scalar-tensor gravity

Fuente: arXiv
Salvato in:
Dettagli Bibliografici
Autori principali: Banerjee, Narayan, Giusti, Andrea, Faraoni, Valerio, Gallerani, Luca, Maltais-Gosselin, Alain
Natura: Preprint
Pubblicazione: 2026
Soggetti:
Accesso online:
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
_version_ 1866917526505521152
author Banerjee, Narayan
Giusti, Andrea
Faraoni, Valerio
Gallerani, Luca
Maltais-Gosselin, Alain
author_facet Banerjee, Narayan
Giusti, Andrea
Faraoni, Valerio
Gallerani, Luca
Maltais-Gosselin, Alain
contents The thermal analogy between the effective fluid of scalar-tensor gravity and Eckart's irreversible thermodynamics is extended to the causal Israel-Stewart model, adopting the minimal ansatz of promoting the heat flux density to a timelike vector. This choice yields analytically manageable constitutive equations, allowing for the first consistent decoupling of the effective temperature $\mathcal{T}$ and the effective thermal conductivity $\mathcal{K}$ of scalar-tensor gravity. Crucially, this new framework preserves the interpretation of general relativity as the equilibrium state approached via a dynamical relaxation process in the vanishing-$\mathcal {KT}$ limit. This new causal formalism is applied to cosmology.
format Preprint
id arxiv_https___arxiv_org_abs_2605_24133
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Towards a causal effective thermodynamics of scalar-tensor gravity
Banerjee, Narayan
Giusti, Andrea
Faraoni, Valerio
Gallerani, Luca
Maltais-Gosselin, Alain
General Relativity and Quantum Cosmology
83D05, 80A17
The thermal analogy between the effective fluid of scalar-tensor gravity and Eckart's irreversible thermodynamics is extended to the causal Israel-Stewart model, adopting the minimal ansatz of promoting the heat flux density to a timelike vector. This choice yields analytically manageable constitutive equations, allowing for the first consistent decoupling of the effective temperature $\mathcal{T}$ and the effective thermal conductivity $\mathcal{K}$ of scalar-tensor gravity. Crucially, this new framework preserves the interpretation of general relativity as the equilibrium state approached via a dynamical relaxation process in the vanishing-$\mathcal {KT}$ limit. This new causal formalism is applied to cosmology.
title Towards a causal effective thermodynamics of scalar-tensor gravity
topic General Relativity and Quantum Cosmology
83D05, 80A17
url https://arxiv.org/abs/2605.24133