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Alternative formulations of the thermodynamics of scalar-tensor theories

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arxiv 2405.20865 v2 pith:A4RYY3PE submitted 2024-05-31 gr-qc math-phmath.MP

classification gr-qcmath-phmath.MP
keywords alternativeeckartfieldfluidformalismformulationsgravityscalar-tensor
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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, upon performing the imperfect fluid decomposition, yields constitutive relations that can be mapped onto Eckart's theory. We then investigate how different couplings to Einstein's gravity, at the level of the field equations, can affect the thermodynamic formalism overall. Last, we specialize the discussion to the case of ``traditional'' scalar-tensor theories and identify a specific choice of the coupling function that leads to a significant simplification of the formalism.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Cosmological constraints and standard sirens forecasts for non-dynamical dark energy in Horndeski gravity

    astro-ph.CO 2026-08 conditional novelty 5.0 of 10

    Standard sirens from third-generation detectors could measure H0 to 0.21% in Extended Cuscuton models, but the forecast omits the modified GW luminosity distance.

  2. Black hole interiors in the thermal view of scalar-tensor gravity

    gr-qc 2025-05 conditional novelty 4.0 of 10

    In the thermal view of Brans-Dicke gravity, black hole singularities are 'hot': the effective temperature KT diverges as 1/t, and a fluid with P=wρ controls whether gravity approaches or departs from general relativity.

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