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

Errata 28/01/2013 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) ...

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.

Damping of visco-resistive Alfven waves in solar spicules

Interaction of Alfven waves with plasma inhomogeneity generates phase mixing which can cause the dissipation of Alfven waves. We investigated the dissipation of standing Alfven waves due to phase mixing at the presence of steady flow and sheared magnetic field in solar spicules. Moreover, the transition region between chromosphere and corona was considered. Our numerical simulation showed that ...

Seismology of solar spicules based on Hinode/SOT observations