Neutrino Emission from Magnetized Microquasar Jets

Figure 2

(a) Pion energy spectra, per p-p collision, obtained for three different incoming fast proton energies ( GeV,  GeV, and  GeV), as a function of the ratio . We consider charged pions () as needed for our purposes in this work. denotes the secondary particle (pion) energy. (b) Variation of the pion injection function, , through the pion energy spectrum, for three different jet densities , located at different points along the model jet axis.

(a)

(b)