Paul Langacker
Published 1998-11-24Version 1
The importance of non-zero neutrino mass as a probe of particle physics, astrophysics, and cosmology is emphasized. The present status and future prospects for the solar and atmospheric neutrinos are reviewed, and the implications for neutrino mass and mixing in 2, 3, and 4-neutrino schemes are discussed. The possibilities for significant mixing between ordinary and light sterile neutrinos are described.
Comments: 16 pages, 2 figures; Invited talk given at 18th International Conference on Neutrino Physics and Astrophysics (NEUTRINO 98), Takayama, Japan, 4-9 Jun 1998
Journal: Nucl.Phys.Proc.Suppl. 77 (1999) 241-256
Implications of Solar and Atmospheric Neutrinos
Implications for CP asymmetries of improved data on $B \to K^0 π^0$
Sensitivity to neutrino decay with atmospheric neutrinos at INO
