Is there supernova evidence for dark energy metamorphosis?

被引:418
作者
Alam, U [1 ]
Sahni, V
Saini, TD
Starobinsky, AA
机构
[1] Inter Univ Ctr Astron & Astrophys, Pune, Maharashtra, India
[2] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[3] LD Landau Theoret Phys Inst, Moscow 119334, Russia
关键词
methods : statistical; cosmological parameters; cosmology : theory;
D O I
10.1111/j.1365-2966.2004.08189.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:275 / 291
页数:17
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