102 citations · 534 across the 14 of their papers we have counts for
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Environmental limits on the non-resonant cosmic-ray current-driven instability
B. Reville, J. G. Kirk, P. Duffy +1
We investigate the so-called non-resonant cosmic-ray streaming instability, first discussed by Bell (2004). The extent to which thermal damping and ion-neutral collisions reduce th…
The transport of cosmic rays in self-excited magnetic turbulence
B. Reville, S. O'Sullivan, P. Duffy +1
The process of diffusive shock acceleration relies on the efficacy with which hydromagnetic waves can scatter charged particles in the precursor of a shock. The growth of self-gene…
Interacting Jets from Binary Protostars
G. C. Murphy, T. Lery, S. O'Sullivan +3
We investigate potential models that could explain why multiple proto-stellar systems predominantly show single jets. During their formation, stars most frequently produce energeti…
A cosmic ray current driven instability in partially ionised media
B. Reville, J. G. Kirk, P. Duffy +1
We investigate the growth of hydromagnetic waves driven by streaming cosmic rays in the precursor environment of a supernova remnant shock. It is known that transverse waves propag…
An explicit scheme for multifluid magnetohydrodynamics
Stephen O'Sullivan, Turlough P. Downes
When modeling astrophysical fluid flows, it is often appropriate to discard the canonical magnetohydrodynamic approximation thereby freeing the magnetic field to diffuse with respe…