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• W2149197860 abstract "We estimate the degree to which the baryon density, $Omega_{b}$, can be determined from the galaxy power spectrum measured from large scale galaxy redshift surveys, and in particular, the Sloan Digital Sky Survey. A high baryon density will cause wiggles to appear in the power spectrum, which should be observable at the current epoch. We assume linear theory on scales $geq 20h^{-1}Mpc$ and do not include the effects of redshift distortions, evolution, or biasing. With an optimum estimate of $P(k)$ to $ksim 2pi/(20 h^{-1} Mpc)$, the $1 sigma$ uncertainties in $Omega_{b}$ are roughly 0.07 and 0.016 in flat and open ($Omega_{0}=0.3$) cosmological models, respectively. This result suggests that it should be possible to test for consistency with big bang nucleosynthesis estimates of $Omega_{b}$ if we live in an open universe." @default.
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• W2149197860 date "1998-03-01" @default.
• W2149197860 modified "2023-09-26" @default.
• W2149197860 title "Determination of the Baryon Density from Large‐Scale Galaxy Redshift Surveys" @default.
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• W2149197860 doi "https://doi.org/10.1086/305284" @default.
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