Extracting Primordial Density Fluctuations
arXiv:astro-ph/9806197 · doi:10.1126/science.280.5368.1405
Abstract
The combination of detections of anisotropy in the Cosmic Microwave Background radiation and observations of the large-scale distribution of galaxies probes the primordial density fluctuations of the universe on spatial scales varying by three orders of magnitude. These data are found to be inconsistent with the predictions of several popular cosmological models. Agreement between the data and the Cold + Hot Dark Matter model, however, suggests that a significant fraction of the matter in the universe may consist of massive neutrinos.
20 pages including 4 color postscript figures. Full-size figures and data compilation available at http://cfpa.berkeley.edu/cmbserve/fluctuations/figures.html
References in corpus (10)
- Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications
- The Age Of Globular Clusters In Light Of Hipparcos: Resolving the Age Problem?
- The Intracluster Gas Fraction in X-ray Clusters : Constraints on the Clustered Mass Density
- A 120-Mpc Periodicity in the Three-Dimensional Distribution of Galaxy Superclusters
- The case against scaling defect models of cosmic structure formation
- Can Baryonic Features Produce the Observed 100 Mpc Clustering?
- What Can Cosmic Microwave Background Observations Already Say About Cosmological Parameters in Open and Critical-Density Cold Dark Matter Models?
- Determination of the Baryon Density from Large Scale Galaxy Redshift Surveys
- Cosmic Strings in an Open Universe: Quantitative Evolution and Observational Consequences
- Arc statistics with realistic cluster potentials. IV. Clusters in different cosmologies
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