The astrophysics of ultrahigh-energy cosmic rays
K Kotera, AV Olinto - Annual Review of Astronomy and …, 2011 - annualreviews.org
The origin of the highest energy cosmic rays is still unknown. The discovery of their sources
is expected to reveal the workings of the most energetic astrophysical accelerators in the …
is expected to reveal the workings of the most energetic astrophysical accelerators in the …
PIC methods in astrophysics: simulations of relativistic jets and kinetic physics in astrophysical systems
Abstract The Particle-In-Cell (PIC) method has been developed by Oscar Buneman, Charles
Birdsall, Roger W. Hockney, and John Dawson in the 1950s and, with the advances of …
Birdsall, Roger W. Hockney, and John Dawson in the 1950s and, with the advances of …
[HTML][HTML] Multidimensional electron beam-plasma instabilities in the relativistic regime
The interest in relativistic beam-plasma instabilities has been greatly rejuvenated over the
past two decades by novel concepts in laboratory and space plasmas. Recent advances in …
past two decades by novel concepts in laboratory and space plasmas. Recent advances in …
Weibel, two-stream, filamentation, oblique, bell, buneman... which one grows faster?
A Bret - The Astrophysical Journal, 2009 - iopscience.iop.org
Many competing linear instabilities are likely to occur in astrophysical settings, and it is
important to assess which one grows faster for a given situation. An analytical model …
important to assess which one grows faster for a given situation. An analytical model …
On electromagnetic instabilities at ultra-relativistic shock waves
M Lemoine, G Pelletier - Monthly Notices of the Royal …, 2010 - academic.oup.com
Recent work on Fermi acceleration at ultra-relativistic shock waves has demonstrated the
need for strong amplification of the background magnetic field on very short scales …
need for strong amplification of the background magnetic field on very short scales …
Multi-scale simulations of particle acceleration in astrophysical systems
This review aims at providing an up-to-date status and a general introduction to the subject
of the numerical study of energetic particle acceleration and transport in turbulent …
of the numerical study of energetic particle acceleration and transport in turbulent …
Weibel instability and associated strong fields in a fully three-dimensional simulation of a relativistic shock
KI Nishikawa, J Niemiec, PE Hardee… - The Astrophysical …, 2009 - iopscience.iop.org
ABSTRACT Plasma instabilities (eg, Buneman, Weibel, and other two-stream instabilities)
excited in collisionless shocks are responsible for particle (electron, positron, and ion) …
excited in collisionless shocks are responsible for particle (electron, positron, and ion) …
On some theoretical problems of laser wake-field accelerators
Enhancement of the quality of laser wake-field accelerated (LWFA) electron beams implies
the improvement and controllability of the properties of the wake waves generated by ultra …
the improvement and controllability of the properties of the wake waves generated by ultra …
Evolution of global relativistic jets: collimations and expansion with kKHI and the Weibel instability
In the study of relativistic jets one of the key open questions is their interaction with the
environment. Here we study the initial evolution of both electron–proton (${e}^{\mbox {--}} …
environment. Here we study the initial evolution of both electron–proton (${e}^{\mbox {--}} …
On Fermi acceleration and magnetohydrodynamic instabilities at ultra-relativistic magnetized shock waves
G Pelletier, M Lemoine… - Monthly Notices of the …, 2009 - academic.oup.com
Fermi acceleration can take place at ultra-relativistic shock waves if the upstream or
downstream magnetic field has been remodelled so that most of the magnetic power lies on …
downstream magnetic field has been remodelled so that most of the magnetic power lies on …