Future Universe With w < -1 Without Big Smash
Srivastava, S. K.
Original · EN
It is demonstrated that if cosmic dark energy behaves like a fluid with equation of state p = w ρ(p and ρ being pressure and energy density respectively) as well as generalized Chaplygin gas simultaneously, Big Rip or Big smash problem does not arise even for equation of state parameter w < -1.Unlike other phantom models, here, scale factor for the future universe is found regular for all time.
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