Massive Neutrinos in Cosmology
arXiv:hep-ph/0511068 · doi:10.1016/j.nuclphysbps.2006.02.002
Abstract
The roles of massive neutrinos in cosmology -- in leptogenesis and in the evolution of mass density fluctuations -- are reviewed. Emphasis is given to the limit on neutrino mass from these considerations.
Plenary talk given at NuFact05, Frascati, 21-26 June 2005
References in corpus (5)
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- The Luminosity and Color Dependence of the Galaxy Correlation Function
- Constraining Neutrino Masses by CMB Experiments Alone
- Weighing Neutrinos with Galaxy Cluster Surveys
- Neutrino Masses from Cosmological Probes
Cited by in corpus (6)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Towards a cosmological neutrino mass detection
- Limit on the Neutrino Mass from the WMAP Three Year Data
- Neutrino masses and beyond-CDM cosmology with LSST and future CMB experiments
- Neutrino Mixings and Leptonic CP Violation from CKM Matrix and Majorana Phases
- Single Field Inflation models allowed and ruled out by the three years WMAP data