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From the 1 of 7 linked papers with an AI index.

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7 papers

astro-ph.HE2026

Self-Consistent Modelling of Neutrino Production in Turbulent Black Hole Coronae

Sébastien Le Bihan, Martin Lemoine, Frank Rieger

The paper presents the hybrid code Turb-AM3, which couples a lepto‑hadronic radiative solver with a stochastic acceleration module to self‑consistently model particle acceleration…

astro-ph.HE2025

Magnetised turbulent plasmas as high-energy particle accelerators

M. Lemoine

This proceedings paper reports on the theoretical modelling of particle acceleration in magnetised turbulent plasmas. It briefly reviews some recent findings obtained from fully ki…

astro-ph.HE2025

Particle acceleration up to the synchrotron burn-off limit in relativistic magnetized turbulence

M. Lemoine, V. Bresci, L. Gremillet

In high-energy astrophysics, interpreting observed spectra hinges on understanding the competition between energy gains and radiative losses. To progress along these lines, we repo…

astro-ph.HE2025

On the origin of ~ 100 TeV neutrinos from the Seyfert galaxy NGC 7469

Qi-Rui Yang, Xiao-Bin Chen, Ruo-Yu Liu +2

The origin of TeV-PeV neutrinos detected by IceCube remains largely unknown. The most significant individual neutrino source is the close-by Seyfert galaxy NGC 1068 at 4.2 leve…

astro-ph.HE2025

Interpreting the multi-TeV emission from GRB 221009A with a second electron component accelerated by turbulence in the jet

Xing-Wei Gong, Ruo-Yu Liu, Ze-Lin Zhang +2

The detection of very high-energy (VHE) afterglow emission of the gamma-ray burst (GRB) 221009A by the Large High Altitude Air Shower Observatory (LHAASO) provides a unique opportu…

physics.plasm-ph2025

Effective theory for stochastic particle acceleration, with application to magnetized turbulence

M. Lemoine

The physics of particle acceleration in turbulent plasmas is a topic of broad interest, which is making rapid progress thanks to dedicated, large-scale numerical experiments. The f…