Stealth scalar fields in dissipative FLRW cosmology obey a generalized Riccati equation with dissipative pressure as driving term, admitting a stable entropy-selected attractor and an unstable repeller that track non-equilibrium evolution to de Sitter.
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Hawking radiation induces a qualitative softening or complete avoidance of the Big Rip singularity in this viscous dark-fluid entropic cosmology.
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Cosmological Stealth fields and Non-Equilibrium thermodynamics
Stealth scalar fields in dissipative FLRW cosmology obey a generalized Riccati equation with dissipative pressure as driving term, admitting a stable entropy-selected attractor and an unstable repeller that track non-equilibrium evolution to de Sitter.
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Singularity softening and avoidance by the action of thermal radiation in a generalized entropic cosmology
Hawking radiation induces a qualitative softening or complete avoidance of the Big Rip singularity in this viscous dark-fluid entropic cosmology.