PPPC 4 DM$\nu$: A Poor Particle Physicist Cookbook for Neutrinos from DM annihilations in the Sun

Understand

We provide ingredients and recipes for computing neutrino signals of TeV-scale Dark Matter annihilations in the Sun.

• For each annihilation channel and DM mass we present the energy spectra of neutrinos at production, including: state-of-the-art energy losses of primary particles in solar matter, secondary neutrinos, electroweak radiation.
• We then present the spectra after propagation to the Earth, including (vacuum and matter) flavor oscillations and interactions in solar matter.
• We also provide a numerical computation of the capture rate of DM particles in the Sun.