We developed this thesis in the context of understanding the interaction of high-energy particles and magnetic fields in extreme astrophysical environments, like pulsars and pulsar wind nebulae. We employed both simulations implemented with the tools currently in development for future gamma-ray data analysis and observations from the LAT instrument onboard the Fermi satellite. In particular, we focused on three sources, the Crab Nebula and pulsar, the supernova remnant SNR G39.2-0.3, and the Westerlund 2 stellar cluster.
| Date of Award | 31 May 2021 |
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| Original language | English |
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| Supervisor | Diego Fernando Torres Ozemo (Director) |
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PLASMA-MAGNETIC FIELD INTERACTION IN EXTREME ASTROPHYSICAL ENVIRONMENTS
Mestre Guillen, E. (Author). 31 May 2021
Student thesis: Doctoral thesis
Mestre Guillen, E. (Author), Torres Ozemo, D. F. (Director),
31 May 2021Student thesis: Doctoral thesis
Student thesis: Doctoral thesis