The identity of dark matter is a question of central importance in both astrophysics and
particle physics. In the past, the leading particle candidates were cold and collisionless, and …

Increasingly stringent limits from LHC searches for new physics, coupled with lack of
convincing signals of weakly interacting massive particle (WIMP) in dark matter searches …

Abstract Particles beyond the Standard Model (SM) can generically have lifetimes that are
long compared to SM particles at the weak scale. When produced at experiments such as …

Current upper bounds on the neutron electric dipole moment constrain the physically
observable quantum chromodynamic (QCD) vacuum angle| θ¯|≲ 10− 11. Since QCD …

We review the theoretical motivations and experimental status of searches for stable
massive particles (SMPs) which could be sufficiently long-lived as to be directly detected at …

An extraordinarily rich zoo of non-baryonic dark matter candidates has been proposed over
the last three decades. Here we present a ten-point test that a new particle has to pass in …

Considering gravitino dark matter scenarios, we obtain the full gauge-invariant result for the
relic density of thermally produced gravitinos to leading order in the standard model gauge …

The IceCube observatory located at the South Pole is a cubic-kilometre optical Cherenkov
telescope primarily designed for the detection of high-energy astrophysical neutrinos …

Considering gravitino dark matter scenarios, we study constraints on the reheating
temperature of inflation. We present the gauge-invariant result for the thermally produced …

If the cosmic dark matter consists of weakly-interacting massive particles, these particles
should be produced in reactions at the next generation of high-energy accelerators …