activity
20052023
most citedPLUTO: a Numerical Code for Computational Astrophysics

1.6k citations · 5k across the 73 of their papers we have counts for

collaborators
Showing 2022Show all

5 papers · 1 filter

astro-ph.IM2022★ 10 cited

A guiding center implementation for relativistic particle dynamics in the PLUTO code

A. Mignone, H. Haudemand, E. Puzzoni

We present a numerical implementation of the guiding center approximation to describe the relativistic motion of charged test particles in the PLUTO code for astrophysical plasma d…

astro-ph.HE2022★ 17 cited

Jet-environment interplay in magnetized binary neutron star mergers

Andrea Pavan, Riccardo Ciolfi, Jay Vijay Kalinani +1

GRB 170817A, the first short gamma-ray burst (sGRB) to be detected in coincidence with a gravitational wave signal, demonstrated that merging binary neutron star (BNS) systems can…

astro-ph.HE2022★ 5 cited

The impact of resistive electric fields on particle acceleration in reconnection layers

E. Puzzoni, A. Mignone, G. Bodo

In the context of particle acceleration in high-energy astrophysical environments featuring magnetic reconnection, the importance of the resistive term of the electric field compar…

astro-ph.HE2022★ 12 cited

A numerical study of the interplay between Fermi acceleration mechanisms in radio lobes of FR-II radio galaxies

Sayan Kundu, Bhargav Vaidya, Andrea Mignone +1

Context: Radio-loud AGNs are thought to possess various sites of particle acceleration, which gives rise to the observed non-thermal spectra. Stochastic turbulent acceleration (STA…

astro-ph.GA2022★ 24 cited

Modelling X-shaped Radio Galaxies: Dynamical and Emission Signatures from the Back-flow model

Gourab Giri, Bhargav Vaidya, Paola Rossi +3

Some of the radio galaxies show distortion in their jets, forming tailed or winged sources. X-shaped radio galaxies are a subclass of winged sources formation mechanism of which is…