Neutrino mass bounds from cosmology
arXiv:hep-ph/0412181 · doi:10.1016/j.nuclphysbps.2005.04.029
Abstract
Cosmology is at present one of the most powerful probes of neutrino properties. The advent of precision data from the cosmic microwave background and large scale structure has allowed for a very strong bound on the neutrino mass. Here, I review the status of cosmological bounds on neutrino properties with emphasis on mass bounds on light neutrinos.
6 pages, 3 figures, talk given at NOW2004 workshop, Conca Specchiulla, Italy, September 11-17, 2004
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- Measurement of the Double Beta Decay Half-life of 150-Nd and Search for Neutrinoless Decay Modes with the NEMO-3 Detector
- Solar mass-varying neutrino oscillations
- Predicting Neutrinoless Double Beta Decay
- Improved Limit on theta_{13} and Implications for Neutrino Masses in Neutrino-less Double Beta Decay and Cosmology
- The discrete flavor symmetry D5
- Neutrinoless Double Beta Decay and Future Neutrino Oscillation Precision Experiments
- Intermediate left-right gauge symmetry, unification of couplings and fermion masses in SUSY
- Confronting mass-varying neutrinos with MiniBooNE
- A Supersymmetric Contribution to the Neutrino Mass Matrix and Breaking of mu-tau Symmetry
- Constraints from neutrino masses and muon (g-2) in the bilinear R-parity violating supersymmetric model
- On Neutrino Oscillations and Time-Energy Uncertainty Relation
- Non-thermal Hot Dark Matter from Inflaton/Moduli Decay: The Momentum Distribution and Relaxing the Cosmological Mass Bound
- Gravitation And the Universe from large Scale-Structures: The GAUSS mission concept
- Flavor Neutrino Oscillations and Time-Energy Uncertainty Relation
- Muon (g-2) from the bulk neutrino field in a warped extra dimensional model