Is there Supernova Evidence for Dark Energy Metamorphosis ?
Ujjaini Alam, Varun Sahni, Tarun Deep Saini, A. A. Starobinsky
Abstract
We reconstruct the equation of state w(z) of dark energy (DE) using a recently released data set containing 172 type Ia supernovae without assuming the prior w(z) ≥ -1 (in contrast to previous studies). We find that dark energy evolves rapidly and metamorphoses from dust-like behaviour at high z (w 0 at z 1) to a strongly negative equation of state at present (w -1 at z 0). Dark energy metamorphosis appears to be a robust phenomenon which manifests for a large variety of SNe data samples provided one does not invoke the weak energy prior ρ+ p ≥ 0. Invoking this prior considerably weakens the rate of growth of w(z). These results demonstrate that dark energy with an evolving equation of state provides a compelling alternative to a cosmological constant if data are analysed in a prior-free manner and the weak energy condition is not imposed by hand.
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