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Effective dissipative cosmology with $Λ$ from the first law of thermodynamics
cosmology-and-nongalactic-astrophysicsgeneral-relativity-and-quantum-cosmologyhigh-energy-physics-phenomenology
We phenomenologically derive a cosmological model that includes both a cosmological constant term $Λ/3$ and a dissipative driving term $β(2 H^{2} + \dot{H})$ by applying both the first law of thermodynamics and an effective entropy (that is proportional to the Bekenstein--Hawking entropy) to matter
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