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AbstractAbstract
[en] Measurements suggest that our universe has a substantial dark energy component. The most recent data on type Ia supernovae give a dark energy density which is in good agreement with other measurements if the dark energy is assumed to be a cosmological constant. Here we examine to what extent that data can put constraints on a more general equation of state for the dark energy
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(c) 2004 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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