Comparing Correlation Lengths of Red and Blue Galaxies: A New Standard Length for Testing Cosmic Isotropy

dc.creatorLongo, Michael J.
dc.date2009-03-10
dc.date.accessioned2026-07-07T12:50:55Z
dc.date.available2026-07-07T12:50:55Z
dc.descriptionI introduce a simple empirical measure of average galaxy cluster sizes based on a comparison of the correlation lengths of red galaxies with blue that can provide a more accurate and bias-free measure of the average size and number density of galaxy clusters. Using 269,000 galaxies from the SDSS DR6 survey, I show that this 3D correlation length, averaged over many clusters, remains very nearly constant at L0= 4.797 +/- 0.024 Mpc/h from small redshifts out to redshifts of 0.5. This serves as a new measure of cosmic length scales and provides a means of testing the standard cosmological model that is almost free of selection biases. The unprecedented accuracy of the technique allows the possibility of sensitive searches for large-scale inhomogeneities. Applying the same technique to the Millennium Simulation galaxies I find very good agreement between it and the SDSS galaxies.
dc.description11 pages
dc.identifierhttps://arxiv.org/abs/0903.1803
dc.identifierhttp://arxiv.org/abs/0903.1803
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/222835
dc.subjectCosmology and Nongalactic Astrophysics
dc.subjectAstrophysics of Galaxies
dc.titleComparing Correlation Lengths of Red and Blue Galaxies: A New Standard Length for Testing Cosmic Isotropy
dc.typetext

Files

Collections