Abstract
I discuss observed and theoretical constraints on the magnetization of gamma-ray burst (GRB) jets. Then, I describe a model based on the striped wind, and I explain how this model can help in solving the photon production problem in photospheric emission models of GRBs.
| Original language | English |
|---|---|
| Journal | Proceedings of Science |
| Volume | 2017-October |
| State | Published - 2017 |
| Externally published | Yes |
| Event | 7th International Fermi Symposium, IFS 2017 - Garmisch-Partenkirchen, Germany Duration: 15 Oct 2017 → 20 Oct 2017 |
Bibliographical note
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