The nature of Dark Matter is still an open problem. One of the well known solution at TeV scale is WIMP scenario. There are three main methods employed in WIMPs' searches: using colliders, direct detection with nuclei and indirectly from astrophysical targets. The first purpose of my McS Project is to contribute to the creation of a portal (gDM bounds) that collect experimental limits and graphically handle them. Secondly, but not less important, we want to compare standard PPPC model prediction for gamma-ray spectra, with the recently published cosmiXs spectra.

gDM bounds - A portal to handle experimental limits on particle dark matter searches

DE CARIA, MICHELA
2023/2024

Abstract

The nature of Dark Matter is still an open problem. One of the well known solution at TeV scale is WIMP scenario. There are three main methods employed in WIMPs' searches: using colliders, direct detection with nuclei and indirectly from astrophysical targets. The first purpose of my McS Project is to contribute to the creation of a portal (gDM bounds) that collect experimental limits and graphically handle them. Secondly, but not less important, we want to compare standard PPPC model prediction for gamma-ray spectra, with the recently published cosmiXs spectra.
2023
gDM bounds - A portal to handle experimental limits on particle dark matter searche
Dark Matter
WIMPS
MAGIC
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.12608/75519