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相关论文: Peculiar thermal states in the first-order thermod…

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We test ideas of the recently proposed first-order thermodynamics of scalar-tensor gravity using an exact geometry sourced by a conformally coupled scalar field. We report a non-monotonic behaviour of the effective ``temperature of…

广义相对论与量子宇宙学 · 物理学 2024-01-11 Numa Karolinski , Valerio Faraoni

Stealth solutions of scalar-tensor gravity and less-known de Sitter spaces that generalize them are analyzed regarding their possible role as thermal equilibria at non-zero temperature in the new first-order thermodynamics of scalar-tensor…

广义相对论与量子宇宙学 · 物理学 2023-08-02 Serena Giardino , Andrea Giusti , Valerio Faraoni

The first-order thermodynamics of scalar-tensor theory is a novel approach that exploits the intriguing relationship between gravity and thermodynamics to better understand the space of gravity theories. It is based on using Eckart's…

广义相对论与量子宇宙学 · 物理学 2023-08-24 Serena Giardino , Andrea Giusti

Previously, the Einstein equation has been described as an equation of state, general relativity as the equilibrium state of gravity, and $f({\cal R})$ gravity as a non-equilibrium one. We apply Eckart's first order thermodynamics to the…

广义相对论与量子宇宙学 · 物理学 2021-06-09 Valerio Faraoni , Andrea Giusti

We investigate a puzzle in the recent thermodynamics of scalar-tensor gravity, in which general relativity is a zero-temperature state of equilibrium and scalar-tensor gravity is the non-equilibrium configuration of an effective dissipative…

广义相对论与量子宇宙学 · 物理学 2022-05-18 Valerio Faraoni , Théo B. Françonnet

A new thermodynamics of scalar-tensor gravity is applied to spatially homogeneous and isotropic cosmologies in this class of theories and tested on analytical solutions. A forever-expanding universe approaches the Einstein "state of…

广义相对论与量子宇宙学 · 物理学 2022-05-06 Serena Giardino , Valerio Faraoni , Andrea Giusti

We extend to the Horndeski realm the irreversible thermodynamics description of gravity previously studied in "first generation" scalar-tensor theories. We identify a subclass of Horndeski theories as an out-of--equilibrium state, while…

广义相对论与量子宇宙学 · 物理学 2022-06-22 Andrea Giusti , Stefan Zentarra , Lavinia Heisenberg , Valerio Faraoni

A new thermal view of scalar-tensor gravity, in which general relativity is the zero-temperature state of gravity, is applied to the specific subclass of $f(R)$ gravity theories and, specifically, to spatially homogeneous and isotropic…

广义相对论与量子宇宙学 · 物理学 2026-01-27 Valerio Faraoni , Santiago Novoa Cattivelli

Analytical solutions of nonminimally coupled scalar field cosmology corresponding to critical scalar field values constitute a potential challenge to the recent first-order thermodynamics of scalar-tensor gravity (a formalism picturing…

广义相对论与量子宇宙学 · 物理学 2022-07-11 Valerio Faraoni , Pierre-Antoine Graham , Alexandre Leblanc

Brans-Dicke gravity does not always reduce to General Relativity in the limit $\omega\to\infty$ for the coupling constant. This anomalous behavior is examined within the formalism of the first-order thermodynamics of scalar-tensor gravity.…

广义相对论与量子宇宙学 · 物理学 2025-08-04 L. Gallerani , A. Giusti , A. Mentrelli , V. Faraoni

The two-parameter inhomogeneous and time-dependent Pimentel solution of Brans-Dicke theory is analyzed to probe and extend the new thermal view in which General Relativity is the zero-temperature (equilibrium) state of scalar-tensor…

广义相对论与量子宇宙学 · 物理学 2026-01-16 Valerio Faraoni , Nikki Veilleux

The phase space of Bianchi I universes in vacuum Brans-Dicke gravity is analyzed in terms of physical variables. The behaviour of the solutions of the field equations near the fixed points (which are solutions of Einstein gravity) is…

广义相对论与量子宇宙学 · 物理学 2024-05-01 Julien Houle , Valerio Faraoni

We discuss and expand a new approach to the thermodynamics of scalar-tensor gravity and its diffusion toward general relativity (seen as an equilibrium state) proposed in a previous Letter [Phys. Rev. D 103, L121501 (2021)], upon which we…

广义相对论与量子宇宙学 · 物理学 2022-01-05 Valerio Faraoni , Andrea Giusti , Andrea Mentrelli

The extreme Reissner-Nordstr\"om black holes have zero surface gravity. However, a semi-classical analysis seems to be ill-definite for these objects and apparently no notion of temperature exists for them. It is argued here that these…

广义相对论与量子宇宙学 · 物理学 2007-05-23 F. G. Alvarenga , A. B. Batista , J. C. Fabris , G. T. Marques

Temperature effects in a scalar field non-minimally coupled to gravity are investigated. The Thermo Field Dynamics formalism is used. This is a topological field theory that allows us to calculate different effects, such as the…

广义相对论与量子宇宙学 · 物理学 2022-03-22 A. F. Santos , Faqir C. Khanna

We derive the equations of motion for Palatini F(R) gravity by applying an entropy balance law T dS= \delta Q+\delta N to the local Rindler wedge that can be constructed at each point of spacetime. Unlike previous results for metric F(R),…

广义相对论与量子宇宙学 · 物理学 2015-03-17 Goffredo Chirco , Christopher Eling , Stefano Liberati

We delve into the first-order thermodynamics of Horndeski gravity, focusing on spatially flat, homogeneous, and isotropic cosmologies. Our exploration begins with a comprehensive review of the effective fluid representation within viable…

广义相对论与量子宇宙学 · 物理学 2024-06-18 Marcello Miranda , Serena Giardino , Andrea Giusti , Lavinia Heisenberg

We explore alternative formulations of the analogy between viable Horndeski gravity and Eckart's first-order thermodynamics. We single out a class of identifications for the effective stress-energy tensor of the scalar field fluid that,…

广义相对论与量子宇宙学 · 物理学 2024-09-30 Luca Gallerani , Marcello Miranda , Andrea Giusti , Andrea Mentrelli

Induced gravity, defined as a globally scale-invariant ``first-generation'' scalar-tensor theory, is investigated within the framework of the thermodynamics of modified gravity theories. The ``temperature of gravity'' and its evolution…

广义相对论与量子宇宙学 · 物理学 2026-01-27 Andrea Giusti

We consider a novel class of $f(\R)$ gravity theories where the connection is related to the conformally scaled metric $\hat g_{\mu\nu}=C(\R)g_{\mu\nu}$ with a scaling that depends on the scalar curvature $\R$ only. We call them C-theories…

广义相对论与量子宇宙学 · 物理学 2011-02-18 Luca Amendola , Kari Enqvist , Tomi Koivisto
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