Extracting Primordial Density Fluctuations
Eric Gawiser,
Joseph Silk
The combination of detections of anisotropy in 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.
E. Gawiser is at the Department of Physics, University of
California at Berkeley, Berkeley, CA 94720, USA. E-mail:
gawiser{at}astron.berkeley.edu. J. Silk is at the Departments of Physics
and Astronomy and the Center for Particle Astrophysics, University of
California at Berkeley, Berkeley, CA 94720, USA.