Can a late-time cosmological model based on baby universe absorption explain the z-variation of w?
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Can a late-time cosmological model based on baby universe absorption explain the z-variation of w?
Jan Ambjorn, Yoshiyuki Watabiki
AbstractWe point out that a simple late-time cosmological model where our Universe can absorb "baby universes" explains the exponential expansion of our universe without the need of a cosmological constant and leads to a z-dependence of the parameter w(z) in the equation of state. In this model w(z) is less than -1 for z sufficiently large.