Errata 28/01/2013 Fundamentals of Neutrino Physics and Astrophysics

Errata 28/12/2014 Fundamentals of Neutrino Physics and Astrophysics

eqn (2.189) (/ pP −m) γ u(pP) = 0 (/ p−m) γ u(pP) = 0 eqn (2.276) +1 following eqn (2.276) following eqn (2.278) eqn (2.361) −1 transform as transform as (normal ordering is implicitly assumed) eqn (2.378) −1 a parity transformation a passive parity transformation eqn (2.385) −1 The transformation The active transformation eqn (2.404) −1 The transformation The active transformation eqn (2.408) ...

Seismology of solar spicules based on Hinode/SOT observations

Physics and Astrophysics Opportunities with Supernova Neutrinos

Neutrinos emitted from a supernova encode useful information about neutrino physics and astrophysics. Interpreting the neutrino signal depends crucially on understanding neutrino production, flavor mixing during propagation, and detection. In this talk, we review the physics potential of a SN neutrino observation.

Recent Progress in Neutrino Astrophysics

Recent progress in neutrino physics has been rapid, to a large extent thanks to observations of neutrinos produced in astrophysical environments. Here, we review the current standing on such questions as neutrino masses and mixings, focusing mainly on the interplay between neutrino physics, astrophysics and cosmology.

ar X iv : a st ro - p h / 01 06 31 7 v 2 2 2 Ju n 20 01 Bremsstrahlung of Flavor - Degenerate Pairs by Neutrinos in the Nuclear Field

Neutrino bremsstrahlung of flavor-degenerate pairs in the field of a nucleus is of potential importance for neutrino astrophysics and is representative of a class of processes connecting leptonic electroweak sectors to real or virtual photons. We focus on first generation flavor production by both electron and muon neutrinos and present Standard Model cross sections and distributions for lead a...