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 …

New data are reported from the operation of the PICO-60 dark matter detector, a bubble
chamber filled with 36.8 kg of CF 3 I and located in the SNOLAB underground laboratory …

Final results are reported from operation of the PICO-60 C 3 F 8 dark matter detector, a
bubble chamber filled with 52 kg of C 3 F 8 located in the SNOLAB underground laboratory …

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 …

The search for dark matter is one of the hottest topics in Physics today. The fact that about
80% of the matter of the Universe is of unknown nature has triggered an intense …

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 …

Dark matter particles will be captured in neutron stars if they undergo scattering interactions
with nucleons or leptons. These collisions transfer the dark matter kinetic energy to the star …

Neutron stars harbour matter under extreme conditions, providing a unique testing ground
for fundamental interactions. We recently developed an improved treatment of dark matter …

White dwarfs, the most abundant stellar remnants, provide a promising means of probing
dark matter interactions, complimentary to terrestrial searches. The scattering of dark matter …

Dark matter capture and annihilation in the Sun can produce detectable high-energy
neutrinos, providing a probe of the dark matter–proton scattering cross section. We consider …