A Search for Neutrinos from Decaying Dark Matter in Galaxy Clusters and Galaxies with IceCube
A Search for Neutrinos from Decaying Dark Matter in Galaxy Clusters and Galaxies with IceCube
The observed dark matter abundance in the Universe can be explained with non-thermal, heavy dark matter models. In order for dark matter to still be present today, its lifetime has to far exceed the age of the Universe. In these scenarios, dark matter decay can produce highly energetic neutrinos, along …