Disentangling a possible dark matter-induced gamma-ray signal from known astrophysical emitters toward the Galactic Center.
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| Fecha de publicación: | 2016 |
| Objetivos: | The project aims to study the gamma-ray excess at the Galactic Center by modeling diffuse emissions, testing dark matter annihilation and decay scenarios, and exploring astrophysical explanations. It will optimize CTA observation strategies and foster astroparticle physics collaboration in Chile. |
| Instrumento: | Fondecyt de Postdoctorado |
| Año de Inicio/Término: | 2016-2018 |
| Financiamiento/Sponsor: | CONICYT |
| Rol del Usuario: | INVESTIGADOR(A) |
| DOI: |
FONDECYT 3160156 |
| Notas: | Using Fermi-LAT data and CTA simulations, the project will analyze the Galactic Center gamma-ray excess, considering dark matter and astrophysical origins. It aims to improve understanding of dark matter properties, refine observational strategies, and build Chile's astroparticle physics expertise. |