Speaker
Rostom Mbarek
Description
Building on recent advancements in understanding particle transport in magnetized media, we present a first-principles scaling law for the formation of non-thermal tails in particle spectra within mildly and strongly magnetized turbulent plasmas. This scaling is validated using results from kinetic Particle-In-Cell simulations, which show excellent agreement with our theoretical predictions. Finally, we discuss the astrophysical implications of these findings, particularly for the proton spectra in the coronae of supermassive black holes.
| Presenter's Name | Rostom Mbarek |
|---|---|
| Presenter's Email Address | [email protected] |
| Recording Permission | YES |
| Virtual Audience Permission | YES |
| Photography Permission | YES |
Primary author
Rostom Mbarek
Co-author
Sasha Philippov
External references
- 25030150
- af6d2a7e-90b6-4ea2-9678-e77237c8824c
