Plasma Physics for Astrophysics

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Galactic winds driven by cosmic ray streaming (2012, methodology): “This research was supported in the framework of the DFG Forschergruppe 1254 “Magnetization of Interstellar and Intergalactic Media: The Prospects of Low-Frequency Radio Observations”. C.P. gratefully acknowledges financial support of the Klaus Tschira Foundation and would furthermore like to thank K”
The physics of gamma-ray bursts & relativistic jets (2014, background): “Uzdensky, D. A., Kulsrud, R. M., Oct. 2000.”
Star-forming galaxies as the origin of diffuse high-energy backgrounds: gamma-ray and neutrino connections, and implications for starburst history (2014, background): “Instead, the confinement of ∼ 100 PeV cosmic rays may be possible in high redshift starbursts, if the diffusion coefficient around ∼ 100 PeV is sufficiently close to that in the Bohm limit [91].”
Cosmic ray driven outflows in global galaxy disc models (2013, background): “Chemical abundances of CRs tell us their lifetime in the Galactic disc is ∼3 Myr, although rays may enter the halo and re-enter the disc, leading to an overall estimate of ∼20 Myr (Shapiro & Silberberg 1970; Kulsrud 2005).”
Relativistic Jets in Active Galactic Nuclei (2018, background): “These waves are likely to accelerate particles through second order, stochastic processes and mediate a form of local viscosity in the flow (Kulsrud 2004; Stawarz & Petrosian 2008).”