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Three-dimensional simulations of non-resonant streaming instability and particle acceleration near non-relativistic astrophysical shocks
Allard Jan van Marle, Fabien Casse and Alexandre Marcowith Monthly Notices of the Royal Astronomical Society 490(1) 1156 (2019) https://doi.org/10.1093/mnras/stz2624
Core-collapse supernovae as cosmic ray sources
Alexandre Marcowith, Vikram V Dwarkadas, Matthieu Renaud, Vincent Tatischeff and Gwenael Giacinti Monthly Notices of the Royal Astronomical Society 479(4) 4470 (2018) https://doi.org/10.1093/mnras/sty1743
Cosmic ray propagation in sub-Alfvénic magnetohydrodynamic turbulence
Particle spectra and efficiency in nonlinear relativistic shock acceleration – survey of scattering models
Donald C. Ellison, Donald C. Warren and Andrei M. Bykov Monthly Notices of the Royal Astronomical Society 456(3) 3090 (2016) https://doi.org/10.1093/mnras/stv2912
High-Energy Cosmic Ray Self-Confinement Close to Extra-Galactic Sources
A. M. Bykov, A. Brandenburg, M. A. Malkov and S. M. Osipov Space Sciences Series of ISSI, Microphysics of Cosmic Plasmas 47 125 (2013) https://doi.org/10.1007/978-1-4899-7413-6_6
Collisionless Shocks in Partly Ionized Plasma with Cosmic Rays: Microphysics of Non-thermal Components
A. M. Bykov, M. A. Malkov, J. C. Raymond, A. M. Krassilchtchikov and A. E. Vladimirov Space Science Reviews 178(2-4) 599 (2013) https://doi.org/10.1007/s11214-013-9984-7
Microphysics of Cosmic Plasmas
A. M. Bykov, M. A. Malkov, J. C. Raymond, A. M. Krassilchtchikov and A. E. Vladimirov Space Sciences Series of ISSI, Microphysics of Cosmic Plasmas 47 523 (2013) https://doi.org/10.1007/978-1-4899-7413-6_19
Magnetic Fields in Cosmic Particle Acceleration Sources
K. M. Schure, A. R. Bell, L. O’C Drury and A. M. Bykov Space Sciences Series of ISSI, Particle Acceleration in Cosmic Plasmas 45 491 (2012) https://doi.org/10.1007/978-1-4614-6455-6_15
Andrei M. Bykov, Donald C. Ellison and Matthieu Renaud Space Sciences Series of ISSI, Large-Scale Magnetic Fields in the Universe 39 71 (2011) https://doi.org/10.1007/978-1-4614-5728-2_3
Cosmic ray current driven turbulence in shocks with efficient particle acceleration: the oblique, long-wavelength mode instability