Probing large-scale structure with galaxy surveys

Details Probing large-scale structure with galaxy surveys Probing large-scale structure with galaxy surveys

Feb 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..555..201f&link_type=abstract

Cosmology and Particle Physics: CAPP 2000. AIP Conference Proceedings, Volume 555, pp. 201-214 (2001).

Physics

Superclusters, Large-Scale Structure Of The Universe, Cosmology, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies

Scientific paper

In recent years, the framework for a plausible theory of large-scale structure formation has emerged: primordial, quasi-scale-invariant perturbations from inflation, which subsequently grow by gravitational instability in a universe with a substantial component of cold dark matter. In the near future, a new generation of galaxy redshift surveys, along with cosmic microwave background missions and other cosmological probes, will test this structure formation paradigm with unprecedented precision. This talk highlights recent progress and expected future developments in our understanding of large-scale structure and in testing the inflationary scenario for its formation. .

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