Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 354, Issue 1, Pages 275-291Publisher
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2004.08189.x
Keywords
methods : statistical; cosmological parameters; cosmology : theory
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We reconstruct the equation of state w(z) of dark energy (DE) using a recently released data set containing 172 Type Ia supernovae (SNe) without assuming the prior w(z) greater than or equal to-1 (in contrast to previous studies). We find that DE evolves rapidly and metamorphoses from dust-like behaviour at high z (wsimilar or equal to 0 at zsimilar to 1) to a strongly negative equation of state at present (wless than or similar to-1 at zsimilar or equal to 0). DE 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 rho+pgreater than or equal to 0. Invoking this prior considerably weakens the rate of growth of w(z). These results demonstrate that DE 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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