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The Astrophysical Journal Letters, ISSN 1538-4357, 07/2008, Volume 682, Issue 1, pp. L5 - L8
Journal Article
The Astrophysical Journal Letters, ISSN 1538-4357, 01/2008, Volume 673, Issue 1, pp. L39 - L42
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 11/2011, Volume 741, Issue 1, p. 39
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 06/2009, Volume 698, Issue 2, pp. 1523 - 1549
Journal Article
Physical Review Letters, ISSN 0031-9007, 02/2015, Volume 114, Issue 8, p. 085003
We study diffusive shock acceleration (DSA) of protons and electrons at nonrelativistic, high Mach number, quasiparallel, collisionless shocks by means of... 
DRIFT ACCELERATION | PHYSICS, MULTIDISCIPLINARY | SUPERNOVA-REMNANTS | PERPENDICULAR SHOCKS | MAGNETIC-FIELD AMPLIFICATION | SIMULATIONS | ION-ACCELERATION | COSMIC-RAYS | Bells | Supernova remnants | Simulation | Supernovae | Instability | Activation | Acceleration | High Mach number
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 09/2019, Volume 882, Issue 2, p. 142
We present the first realistic 3D simulations of flame front instabilities during type I X-ray bursts. The unperturbed front is characterized by the balance... 
EVOLUTION | ROTATING NEUTRON-STARS | ASTRONOMY & ASTROPHYSICS | hydrodynamics | methods: numerical | instabilities | stars: neutron | X-rays: bursts | PROPAGATION
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 09/2019, Volume 882, Issue 1, p. 3
The self-regulation of cosmic-ray (CR) transport in the interstellar and intracluster media has long been viewed through the lenses of linear and quasi-linear... 
ION-BEAM | COSMIC-RAY PROPAGATION | PITCH-ANGLE SCATTERING | magnetic fields | plasmas | GALACTIC WINDS | IN-CELL SIMULATIONS | DRIVEN | turbulence | instabilities | solar wind | SHOCK ACCELERATION | cosmic rays | WAVE-PARTICLE INTERACTIONS | ASTRONOMY & ASTROPHYSICS | MAGNETIC-FIELD | NONLINEAR ALFVEN WAVES | Physics - High Energy Astrophysical Phenomena
Journal Article
Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 10/2013, Volume 435, Issue 1, pp. L1 - L5
The current state of the art in pulsar magnetosphere modelling assumes the force-free limit of magnetospheric plasma. This limit retains only partial... 
MHD | Relativistic processes | Methods:Numerical | Pulsars:General | relativistic processes | methods: numerical | pulsars: general | ASTRONOMY & ASTROPHYSICS
Journal Article