A. D. Dolgov
Published 2003-06-17Version 1
The bounds on neutrino masses and mixing that follows from the data on light element abundances, large scale structure formation, and angular fluctuations of cosmic microwave background radiation are analyzed. The role of neutrino oscillations in BBN and the bounds on cosmological lepton asymmetry are discussed.
Comments: Talk presented at the NOON 2003 workshop, February 10-14, 2003, Kanazawa, Japan (to be published in the Proceedings), 10 pages
Astrophysical and Cosmological Constraints on Neutrino masses
Particles and the Universe
Cosmological Constraints on the Gravitational Interactions of Matter and Dark Matter
