Eckart heat flux holds for all timelike scalar configurations in F(Φ,X)R + G theories if and only if F_X ≡ 0, reducing the theory to a Jordan-like subclass of Horndeski.
Espinosa-Portal´ es and J
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Proposes primordial black holes from modified small-scale fluctuations and entropic acceleration in expanding spacetime as explanations for dark matter and dark energy.
Holographic duality equates cosmological constant acceleration with de Sitter horizon thermodynamics, extending to time-dependent GREA entropic acceleration when matter is present.
citing papers explorer
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Eckart heat-flux applicability in $F(\Phi,X)R$ theories and the existence of temperature gradients
Eckart heat flux holds for all timelike scalar configurations in F(Φ,X)R + G theories if and only if F_X ≡ 0, reducing the theory to a Jordan-like subclass of Horndeski.
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Beyond the Standard Model of Cosmology: Testing new paradigms with a Multiprobe Exploration of the Dark Universe
Proposes primordial black holes from modified small-scale fluctuations and entropic acceleration in expanding spacetime as explanations for dark matter and dark energy.
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GREA and Dark Energy: A holographic correspondence
Holographic duality equates cosmological constant acceleration with de Sitter horizon thermodynamics, extending to time-dependent GREA entropic acceleration when matter is present.