why streams of energy-matter are emited along the axis of rotation of a compact object? (or) what is the reason that they are emited along the axis of rotation of a compact object?
How are they formed? And why are they so bright?
In the literature one often finds covariant relativistic generalizations of classical non equilibrium statistical equations (Boltzmann, Vlasov, Landau, fokker-planck, etc...) but I wonder what is the ...
what is the simplest way to understand the physics of relativistic jets? we know that they have axial symmetry with very tight angular spread, presumably aligned with the axis of rotation of the ...