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Observational constraints on low redshift evolution of dark energy: How consistent are different observations?
PHYSICAL REVIEW D, no. 10 (2005)
摘要
The dark energy component of the Universe is often interpreted either in terms of a cosmological constant or as a scalar field. A generic feature of the scalar field models is that the equation of state parameter w equivalent to P/rho for the dark energy need not satisfy w=-1 and, in general, it can be a function of time. Using the Markov...更多
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