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Thermal origin of the attractor-to-general-relativity in scalar-tensor gravity
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The convergence of scalar-tensor gravity to general relativity, or the departure from it, are described in a new analogy with heat dissipation in a viscous fluid. This new thermal picture is applied to cosmology, shedding light on whether gravity deviates from general relativity early on and approaches it later in the cosmic history.
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Cited by 3 Pith papers
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Gravitational Waves as Thermodynamic Shear Excitations in Scalar-Tensor Gravity
In scalar-tensor gravity, a transverse-traceless gravitational wave performs gauge-invariant shear work on the scalar-field fluid, with power = (KT/4) times the squared strain rate.
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Towards a causal effective thermodynamics of scalar-tensor gravity
Extends scalar-tensor gravity thermodynamics to causal Israel-Stewart model via timelike heat flux ansatz, decoupling T and K while preserving GR equilibrium.
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Black hole interiors in the thermal view of scalar-tensor gravity
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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