Update on work underway and planned at Boulby underground Laboratory. In particular Dark Matter related studies
In this talk, I will present the phenomenology of dark-matter production in the case where it is both produced by thermal processes and by the evaporation of primordial black holes. I will show how the evaporation of primordial black holes may dramatically affect the production of dark-matter particles as well as its phase-space distribution. I will also show that the population of DM...
Liquid xenon time projection chambers (LXe-TPCs) have set leading limits on dark matter scattering over the past two decades. These have so far employed low-background photomultiplier tubes to detect the xenon VUV luminescence. With SiPMs now yielding competitive photon detection performance in the VUV, the possibility of using this technology in the next generation of experiments is becoming...
We discuss PBHs as dark matter, including not only in galaxies and clusters of galaxies but extremely massive PBHs which may allow the total entropy to reach the maximum holographic value
We report on the first 15 months of the QSHS project, an STFC funded collaboration building a UK based apparatus searching for wave-like dark matter in our galactic halo.
We will discuss an experiment for searching axions and axion-like-particles in the galactic halo using quantum-enhanced interferometry. This setup will search for axions in the mass range from 10−16 eV up to 10−12 eV using an optical cavity. The sensitivity will be enhanced using squeezed states of light similar to the gravitational-wave detectors. The proposed experiment has the potential to...
The QSNET consortium is building a UK network of next-generation atomic and molecular clocks that will achieve unprecedented sensitivity in testing variations of the fine structure constant, alpha , and the electron-to-proton mass ratio, μ. In the range of parameters probed, either we will discover new physics, or we will impose new constraints on violations of fundamental symmetries and a...