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- W1574244493 abstract "We examine the cosmic microwave background (CMB) anisotropy for signatures of early quintessence dark energy -- a non-negligible quintessence energy density during the recombination and structure formation eras. In contrast to a $Lambda$CDM cosmology, early quintessence leads to a larger suppression of structure growth. Because of this influence on the clustering of dark matter and the baryon-photon fluid, we may expect to find trace signals in the CMB and the mass fluctuation power spectrum. In detail, we demonstrate that suppressed clustering power on small length-scales, as suggested by the combined Wilkinson Microwave Anisotropy Probe (WMAP) / CMB / large scale structure data set, is characteristic of early quintessence." @default.
- W1574244493 created "2016-06-24" @default.
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- W1574244493 date "2003-10-15" @default.
- W1574244493 modified "2023-10-17" @default.
- W1574244493 title "Early Quintessence and the CMB" @default.
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- W1574244493 hasPublicationYear "2003" @default.
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