A barotropic fluid with pressure p=ρ[ζ0+ζ1(t-t0)^-2n] yields an exact non-singular bouncing FLRW solution with late-time acceleration.
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Modeling a Non-Singular Universe with Late-Time Acceleration through a Novel Inhomogeneous Barotropic Equation of State
A barotropic fluid with pressure p=ρ[ζ0+ζ1(t-t0)^-2n] yields an exact non-singular bouncing FLRW solution with late-time acceleration.