Neutron EDM constrains direct dark matter detection prospects

Tensor Detection Severely Constrains Axion Dark Matter

Prospects for direct dark matter detection in the Constrained MSSM

We outline the WIMP dark matter parameter space in the Constrained MSSM by performing a comprehensive statistical analysis that compares with experimental data predicted superpartner masses and other collider observables as well as a cold dark matter abundance. We include uncertainties arising from theoretical approximations as well as from residual experimental errors on relevant Standard Mode...

WIMP Dark Matter Direct Detection

D. Bauer, A. Borgland, B. Cabrera, F. Calaprice, J. Cooley, P. Cushman, T. Empl, R. Essig, E. Figueroa-Feliciano, R. Gaitskell, C. Galbiati, S. Golwala, J. Hall, R. Hill, A. Hime, E. Hoppe, L. Hsu, E. Hungerford, R. Jacobsen, M. Kelsey, R. F. Lang, W. H. Lippincott, B. Loer, S. Luitz, V. Mandic, J. Mardon, J. Maricic, R. Maruyama, D. N. McKinsey, R. Mahapatra, H. Nelson, J. Orrell, K. Palladino...

Direct detection prospects of dark vectors with xenon-based dark matter experiments

Dark matter experiments primarily search for the scattering of WIMPs on target nuclei of well shielded underground detectors. The results from liquid scintillator experiments furthermore provide precise probes of very light and very weakly coupled particles that may be absorbed by electrons. In these proceedings we summarize previously obtained constraints on long-lived dark matter vector parti...

Direct detection of galactic halo dark matter.

The Milky Way galaxy contains a large, spherical component which is believed to harbor a substantial amount of unseen matter. Recent observations indirectly suggest that as much as half of this "dark matter" may be in the form of old, very cool white dwarfs, the remnants of an ancient population of stars as old as the galaxy itself. We conducted a survey to find faint, cool white dwarfs with la...