Magnetic fields in the universe : from laboratory and stars to primordial structures, Angra dos Reis, Brazil, 28 November - 3 December 2004

By E. Pino, G. Lugones, A. Lazarian. 2005

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Short-hard gamma-ray bursts (2007, methodology): “It is also higher than estimates of the SHB rate that were done before the detection of SHB afterglows (Schmidt, 2001; Ando, 2004; Guetta & Piran, 2005) by a factor of 10 − 100.”
Acceleration of primary and secondary particles in galaxy clusters by compressible MHD turbulence: from radio haloes to gamma-rays (2010, background): “As a particle bounces back and forth between converging magnetic fluxes, it gains energy through the first order Fermi acceleration (de Gouveia dal Pino & Lazarian 2003, 2005; see also Lazarian 2005).”
MHD simulations of the magnetorotational instability in a shearing box with zero net flux - I. The issue of convergence (2007, methodology): “We note that there is no reason why this state of af-fairs should not apply when using Godunov codes like ATHENA (Gardiner & Stone 2005a) or RAMSES (Teyssier 2002; Fromang et al. 2006) or other codes making use of hy-perviscosity to stabilise the numerical scheme, like the PENCIL code (Brandenburg…”