Summary

2000/08/31 by John Ellis
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #Neutrino Physics Research #hep-ph

paper · pdf · doi:10.1016/s0920-5632(00)00981-6

published as Nucl.Phys.Proc.Suppl.91:503-516,2001 · 15 pages, 12 eps figures, uses espcrc2.sty

arxiv created 2000/08/31 · openalex publication_date 2001/01/01 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

Aspects of neutrino physics beyond the Standard Model are emphasized, including the emerging default options for atmospheric and solar neutrino oscillations, namely nu_mu to nu_tau and nu_e to nu_mu,tau respectively, and the need to check them, the prospects opened up by the successful starts of SNO and K2K, the opportunities for future long-baseline neutrino experiments and high-energy astrophysical neutrinos. Finally, comments are made on the road map for realizing the exciting physics potential of neutrino factories.

Citations

• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Can neutrinos be degenerate in mass?
• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• The atmospheric neutrino flavor ratio from a 3.9 fiducial kiloton-year exposure of Soudan 2
• A flat Universe from high-resolution maps of the cosmic microwave background radiation
• Neutrino oscillation physics with a neutrino factory
• The Sudbury Neutrino Observatory