High Energy Neutrino Emission from Astrophysical Jets in the Galaxy

Table 1

Values of various physical and model parameters pertaining to the -ray emission from the jet, for the simulation run, obtained with the linear method and the Hancock integrator.

Parameter		Comments
Cell size (×10^10 cm)	0.25	PLUTO's computational cell
(cm^−3)		Initial jet matter density
(cm^−3)		Stellar wind density
(cm^−3)		Accretion disk wind density
(s)		Model execution time
Interpolation method	Linear
Integrator	MUSCL-Hancock
EOS	Ideal	Equation of state
BinSep (cm)		Binary star separation
/	3–10	Mass range of collapsed star
/	10–30	Mass range of main Seq. star
	0.26	Initial jet speed
		Jet kinetic luminosity
		Fast proton energy fraction
		Neutrino energy fraction (from fast protons)
		Fast proton power law index
(GeV)		Cutoff energy of the fast proton distribution
Grid resolution	120 200 120	PLUTO grid resolution ()