Particle physics today faces the challenge of explaining the mystery of dark matter, the origin
of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent …

Indirect searches for dark matter are based on detecting an anomalous flux of photons,
neutrinos or cosmic-rays produced in annihilations or decays of dark matter candidates …

The observation of electromagnetic radiation from radio to γ-ray wavelengths has provided a
wealth of information about the Universe. However, at PeV (10 15 eV) energies and above …

Weakly interacting massive particles (WIMPs) have long reigned as one of the leading
classes of dark matter candidates. The observed dark matter abundance can be naturally …

Neutron stars close to the Galactic center are expected to swim in a dense background of
dark matter. For models in which the dark matter has efficient interactions with neutrons, they …

While astrophysical and cosmological probes provide a remarkably precise and consistent
picture of the quantity and general properties of dark matter, its fundamental nature remains …

Neutron stars provide a cosmic laboratory to study the nature of dark matter particles and
their interactions. Dark matter can be captured by neutron stars via scattering, where kinetic …

The combination of the high intensity proton beam facilities and massive detectors for
precision measurements of neutrino oscillation parameters including the charge-parity …

Exploring dark matter via observations of extreme astrophysical environments--defined here
as heavy compact objects such as white dwarfs, neutron stars, and black holes, as well as …

The Sun provides an excellent target for studying spin-dependent dark matter-proton
scattering due to its high matter density and abundant hydrogen content. Dark matter …