Building: 31 (Physik Ost)
Room: 02.012
E-mail: laura.eisenberger@stud-mail.uni-wuerzburg.de
Goal: GHz to TeV prediction of primary (prompt, decay/annihilation), secondary (Inverse Compton, synchrotron), and tertiary emission (secondary annihilation to photons) from scotogenic dark matter models.
Methods: Spectral modelling, energy losses, particle propagation, line-of-sight integration, multiwavelength data comparison.
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