CORDIS Project
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The GR-PLUTO project investigates magnetic reconnection in relativistic plasmas around black holes using advanced numerical simulations. By implementing a non-constant resistivity in general relativistic magnetohydrodynamic models, it aims to enhance our understanding of particle acceleration and magnetic dissipation i…
Magnetic fields shape the dynamics of relativistic plasmas that orbit around astrophysical black holes (BHs), as observed in current general relativistic magnetohydrodynamic (GRMHD) models.
A primary example is magnetic reconnection, i.e. the rearrangement of the structure of magnetic field lines, which converts magnetic energy into kinetic and thermal energy and accelerates particles to relativistic velocities, thus producing the high-energy non-thermal radiation observed from accreting compact…
UNIVERSITA DEGLI STUDI DI TORINO
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