The IceCube collaboration has observed the first steady-state point source of high-energy
neutrinos, coming from the active galaxy NGC 1068. If neutrinos interacted strongly enough …

We constrain the neutrino-dark matter cross section using properties of the dark matter
density profiles of Milky Way dwarf spheroidal galaxies. The constraint arises from core …

The detectability of light dark matter in direct detection experiments is limited by the small
kinetic energy of the recoiling targets. Thus, scenarios where dark matter is boosted to …

Elastic collisions with relativistic electrons from the blazar's jet can accelerate dark matter
(DM) particles in the DM spike surrounding the supermassive black hole at its center. This …

Cosmic ray (CR) upscattering of dark matter is considered as one of the most straightforward
mechanisms to accelerate ambient dark matter, making it detectable at high threshold, large …

A bstract Discrete flavor symmetries have been an appealing approach for explaining the
observed flavor structure, which is not justified in the Standard Model (SM). Typically, these …

We probe dark matter-electron scattering using high-energy neutrino observations from the
Sun. Dark matter (DM) interacting with electrons can get captured inside the Sun. These …

We search for energetic electron recoil signals induced by boosted dark matter (BDM) from
the galactic center using the COSINE-100 array of NaI (Tl) crystal detectors at the Yangyang …

Diffuse neutrinos from past supernovae in the Universe present us with a unique opportunity
to test dark matter (DM) interactions. These neutrinos can scatter and boost the DM particles …

We demonstrate that ionization of H 2 by dark matter in dense molecular clouds can provide
strong constraints on the scattering strength of dark matter with electrons. Molecular clouds …