no code implementations • 8 Sep 2020 • Xavier Rodrigues, Simone Garrappa, Shan Gao, Vaidehi S. Paliya, Anna Franckowiak, Walter Winter
We find two hadronic models that can describe the multi-wavelength emission during all three states: a leptohadronic model with a contribution from photo-hadronic processes to X-rays and gamma rays, and a proton synchrotron model, where the emission from keV to 10 GeV comes from proton synchrotron radiation.
High Energy Astrophysical Phenomena
1 code implementation • 16 Apr 2019 • Leonel Morejon, Anatoli Fedynitch, Denise Boncioli, Daniel Biehl, Walter Winter
However, the interactions of nuclei above the pion production threshold are commonly modeled by treating the nucleus as a superposition of free nucleons -- ignoring the effect of the nuclear medium.
High Energy Astrophysical Phenomena Nuclear Theory
1 code implementation • 10 Jan 2019 • Jonas Heinze, Anatoli Fedynitch, Denise Boncioli, Walter Winter
Better constrained parameters include the maximal rigidity and the mass composition at the source.
High Energy Astrophysical Phenomena
