2003/10/14 by William J. Marciano, William J Marciano, Zohreh Parsa · 96 citations
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #Electroweak interaction #Elementary particle #Neutrino #Neutrino Physics Research #Neutrino oscillation #Particle physics theoretical and experimental studies #Scattering #Standard Model (mathematical formulation) #Sterile neutrino #Symmetry breaking #hep-ph
paper · pdf · doi:10.1088/0954-3899/29/11/013
published in Journal of Physics G Nuclear and Particle Physics 29(11), 2629-2645 (IOP Publishing) · 20 pages, published in Particle and Nuclear Physics Journal G (Nov 2003)
openalex publication_date 2003/10/14 · arxiv created 2004/03/15 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06
Standard model predictions for neutrino–electron scattering cross-sections, including effects of electroweak radiative corrections, are reviewed. The sensitivity of these quantities to neutrino dipole moments, Z ′ bosons and dynamical symmetry breaking is described. Neutrino indices of refraction in matter are also discussed. A perspective on future initiatives with intense neutrino sources, such as from stopped pion decays at a neutron spallation source, superbeams or neutrino factories, is given.