Dark matter is one of the greatest unsolved mysteries in cosmology at the present time.
About 80% of the Universe′ s gravitating matter is nonluminous, and its nature and …

We review the phenomenology of models with flat, compactified extra dimensions where all
of the Standard Model fields are allowed to propagate in the bulk, known as Universal Extra …

We use ATLAS and CMS searches in the monojet+ missing energy and monophoton+
missing energy final state to set limits on the couplings of dark matter to quarks and gluons …

Dark matter pair production at high energy colliders may leave observable signatures in the
energy and momentum spectra of the objects recoiling against the dark matter. We use LEP …

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 …

With much higher sensitivities due to coherence effects, it is often assumed that the first
evidence for direct dark matter detection will come from experiments probing spin …

XENON10 is an experiment to directly detect weakly interacting massive particles (WIMPs),
which may comprise the bulk of the nonbaryonic dark matter in our Universe. We report new …

The Korea Invisible Mass Search (KIMS) experiment presents new limits on WIMP-nucleon
cross section using the data from an exposure of 3409 kgd taken with low background CsI …

Bubble chambers were the dominant technology used for particle detection in accelerator
experiments for several decades, eventually falling into disuse with the advent of other …

The PICASSO experiment at SNOLAB reports new results for spin-dependent WIMP
interactions on 19F using the superheated droplet technique. A new generation of detectors …