activity
20052024
most citedAn HLLC Riemann Solver for Relativistic Flows: I. Hydrodynamics

224 citations · 524 across the 11 of their papers we have counts for

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Showing astro-ph.HEShow all

8 papers · 1 filter

astro-ph.HE2024★ 10 cited

Relativistic reconnection with effective resistivity: I. Dynamics and reconnection rate

M. Bugli, E. F. Lopresti, E. Figueiredo +6

Relativistic magnetic reconnection is one of the most fundamental mechanisms considered responsible for the acceleration of relativistic particles in astrophysical jets and magneto…

astro-ph.HE2024

Evolution of current and pressure driven instabilities in relativistic jets

M. Musso, G. Bodo, G. Mamatsashvili +2

Instabilities in relativistic magnetized jets are thought to be deeply connected to their energy dissipation properties and to the consequent acceleration of the non-thermal emitti…

astro-ph.HE2016★ 29 cited

Linear stability analysis of magnetized jets: the rotating case

G. Bodo, G. Mamatsashvili, P. Rossi +1

We perform a linear stability analysis of magnetized rotating cylindrical jet flows in the approximation of zero thermal pressure. We focus our analysis on the effect of rotation o…

astro-ph.HE2014★ 12 cited

Linear and nonlinear evolution of current-carrying highly magnetized jets

M. Anjiri, A. Mignone, G. Bodo +1

We investigate the linear and nonlinear evolution of current-carrying jets in a periodic configuration by means of high resolution three-dimensional numerical simulations. The jets…

astro-ph.HE2014★ 36 cited

On the convergence of Magnetorotational turbulence in stratified isothermal shearing boxes

G. Bodo, F. Cattaneo, A. Mignone +1

We consider the problem of convergence in stratified isothermal shearing boxes with zero net magnetic flux. We present results with the highest resolution to-date--up to 200 grid-p…

astro-ph.HE2013★ 68 cited

Linear stability analysis of magnetized relativistic jets: the nonrotating case

G. Bodo, G. Mamatsashvili, P. Rossi +1

We perform a linear analysis of the stability of a magnetized relativistic non-rotating cylindrical flow in the aproximation of zero thermal pressure, considering only the m = 1 mo…