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- W2036065650 abstract "We test models for the cosmic inhomogeneity spectrum based on cold dark matter against the angular correlation function, the statistics of temperature maxima and minima and the quadrupole amplitude in COBE-DMR maps. We show that while pure CDM and shallow CDM + string models are not completely consistent with COBE's data, steeper spectra provided by texture or isocurvature models pass the correlation-function and peak-number tests for practically any value of the cosmic density parameter including Ω0 = 1. CDM + texture models with Ω0 ⋍ 0.7 also allow to reduce the well-known quadrupole discrepancy, and provide good fits with the best bias factor favored by recent measurement and a Hubble constant H0 ⋍ 70 km s−1 Mpc−1 for the resulting value of Ω0h they also agree with the properties of galaxy distributions. We suggest that a spectrum like the texture one and steeper than pure CDM can link the 10 Mpc and 103 Mpc regions and solve the problems of the cold matter scenario." @default.
- W2036065650 created "2016-06-24" @default.
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- W2036065650 date "1996-12-01" @default.
- W2036065650 modified "2023-09-28" @default.
- W2036065650 title "Tests for cosmic dark matter from COBE" @default.
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- W2036065650 doi "https://doi.org/10.1016/s0927-6505(96)00039-4" @default.
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