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Particle acceleration via magnetic reconnection in large-scale MHD jet simulations

Published online by Cambridge University Press:  11 September 2023

Matteo Nurisso
Affiliation:
SISSA, Via Bonomea 265, I-34136 Trieste, Italy
Annalisa Celotti
Affiliation:
SISSA, Via Bonomea 265, I-34136 Trieste, Italy NAF - Osservatorio Astronomico di Brera, Via Bianchi 46, I-23807 Merate Italy, INFN - Via Valerio 2, I-34127 Trieste, Italy
Andrea Mignone
Affiliation:
Dipartimento di Fisica Generale, Universitá di Torino, Via Pietro Giuria 1, I-10125 Torino, Italy
Gianluigi Bodo
Affiliation:
INAF - Osservatorio Astrofisico di Torino, Strada Osservatorio 20, I-10025 Pino Torinese, Italy
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Abstract

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We present a new algorithm for the identification and physical characterization of current sheets and reconnection sites as well as the update of post-reconnection particles spectra in 2D and 3D large scale relativistic magnetohydrodynamic simulations. Lagrangian particles, which follow the fluid, are used to sample plasma parameters before entering the reconnection sites that form during the evolution of the different configurations considered. With the sampled parameters and a subgrid model based on results of Particle-in-Cell simulations we introduced in the PLUTO code an algorithm able to describe the post-reconnection spectra associated to the non-thermal component.

Type
Poster Paper
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

References

Nurisso, M., Celotti, A., Mignone, A., Bodo, G., 2023, MNRAS, 522, 5517 CrossRefGoogle Scholar
Nurisso, M., Celotti, A., Mignone, A., Bodo, G., 2023 In preparation Google Scholar