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- W2039536400 abstract "Prompted by the recent MAXIMA-1 and BOOMERANG-98 measurements of the cosmic microwave background (CMB) anisotropy power spectrum, and motivated by the results from the observation of high-redshift Type Ia supernovae, we investigate CMB anisotropies in quintessence models in order to characterize the nature of the dark energy today. We perform a Bayesian likelihood analysis, using the MAXIMA-1 and BOOMERANG-98 published bandpowers, in combination with COBE/DMR, to explore the space of quintessence parameters: the quintessence energy density Omega_phi and equation of state w_phi. We restrict our analysis to flat, scale-invariant, inflationary adiabatic models. We find that this simple class of inflationary models, with a quintessence component Omega_phi < ~0.7, -1 < = w_phi < ~-0.5, is in good agreement with the data. Within the assumptions of our analysis, pure quintessence models seem to be slightly favored, although the simple cosmological constant scenario is consistent with the data." @default.
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- W2039536400 date "2001-02-01" @default.
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- W2039536400 title "Implications for Quintessence Models from MAXIMA-1 and BOOMERANG-98" @default.
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- W2039536400 doi "https://doi.org/10.1086/318904" @default.
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