Future universe with w<−1 without big smash

It is demonstrated that if cosmic dark energy behaves like a fluid with equation of state p=wρ (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, the scale factor for the future universe is found regular for all time.