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- W2042484553 abstract "We consider constraints on the structure formation model based on non-Gaussian fluctuations generated during inflation, which have distributions. Using three data sets, the abundance of the clusters at z=0, moderate z and the correlation length, we show that constraints on the non-Gaussianity and the amplitude of fluctuations and the density parameter can be obtained. We obtain an upper bound forΩm, and a lower bound for the non-Gaussianity and the amplitude of the fluctuations. Using the abundance of clusters at z∼0.6, for the spectrum parametrized by cold dark matter (CDM) shape parameter Γ=0.23, we obtain an upper bound for the density parameter of Ωm∼0.5 and lower bounds for the amplitude of σ8∼0.7 and for the non-Gaussianity of fluctuations ofG∼2 (m∼200), where G=1 for Gaussian." @default.
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- W2042484553 date "1999-12-01" @default.
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- W2042484553 title "Constraints on a non-Gaussian χm2 cold dark matter model" @default.
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- W2042484553 doi "https://doi.org/10.1046/j.1365-8711.1999.03033.x" @default.
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