Supernova Neutrinos
Petr Vogel
Abstract
I describe how the signals corresponding to the supernova νe and νe (charged current reactions) as well as all active neutrinos (neutral current reactions) can be separately observed in various existing detectors. These observations would make it possible to determine the flux and average energy (or temperature) for each of these three neutrino signal components. I argue that all these quantities are needed in order to understand the interplay between the so far poorly known supernova neutrino emission process and the neutrino oscillations.
Create a lesson
Related papers
6He structure from semiclassical 3D models based on ab initio spatial correlations
Mengyao Huang, Tobias Frederico, Peng Yin et al.
Algebraic coefficients of fractional parentage for three particles in the oscillator Jacobi basis
A. Stepšys, S. Mickevičius, D. Germanas
Effective shear viscosity from the friction term in relativistic multi-fluid hydrodynamics
Christian Spieles, Marcus Bleicher
Four-dimensional QCD equation of state with a critical surface from contours of constant entropy density
Tristan Gyure, Hitansh Shah, Lorenzo Formaggio et al.
Prospects for modelling odd and odd-odd nuclei using energy density functionals
A. V. Afanasjev, B. Bally, M. Bender et al.
Fast Monte Carlo calculation of multiple scattering in resonant neutron capture
R. M. Djilkibaev