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Future Universe With w < -1 Without Big Smash | | S.K.Srivastava
; | | Date: |
2 Jul 2004 | | Journal: | Phys.Lett. B619 (2005) 1-4 DOI: 10.1016/j.physletb.2005.05.056 | | Subject: | astro-ph gr-qc | | Abstract: | It is demonstrated that if cosmic dark energy behaves like a fluid with equation of state $p = {
m w}
ho (p$ and $
ho$ 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 ${
m w} < -1$.Unlike other phantom models, here, scale factor for the future universe is found regular for all time. | | Source: | arXiv, astro-ph/0407048 | | Services: | Forum | Review | PDF | Favorites | |
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