2003/10/06 by Steen Hannestad, Hannestad, Steen
Physics and Astronomy · #Astrophysics (astro-ph) #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #astro-ph #hep-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0310133
15 pages, 5 figures, invited talk given at Beyond the Desert '03, Ringberg, 11-15 July 2003
arxiv created 2003/10/06 · openalex publication_date 2003/10/06 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Cosmological observations have in the past few years become an increasingly powerful method for determining parameters within the neutrino sector, such as the presence of sterile states and the mass of neutrinos. I review the current status of the field in light of recent measurements of the cosmic microwave background by the WMAP collaboration, as well as current large scale galaxy surveys.