Rather than executing full-cascade simulations, we employ ana- lytic approximations to compute multi-messenger yields

Particle trajectories, multi-messenger interaction efficiency Under this magnetic configuration, cosmic-ray proton transport is governed by the Lorentz force,d⃗ p/dt= q( ⃗β× ⃗B)

1 Pith paper cite this work. Polarity classification is still indexing.

1 Pith paper citing it