KM3NeT upper bounds of detection rates of solar neutrinos from annihilations of dark matter at the solar core

The Weakly Interacting Massive Particles (WIMPs) so far remain one of the most popular candidates for dark matter. If captured gravitationally inside core Sun, these WIMPs may produce high-energy neutrinos as end product in case they undergo self-annihilations at solar core. In this work, we address detectability such proposed KM3NeT detector. Upper bounds detection rate are computed a generic matter scenario and also when specific models particle chosen. upper muon event rates different annihilating masses each cases annihilation channels (e.g. [Formula: see text], etc.). These by considering scattering cross-section using obtained from PandaX-4T direct search experiment.