Directional dark matter detection beyond the neutrino bound
Physical Review D Particles Fields Gravitation and Cosmology 90:5 (2014)
Abstract:
Coherent scattering of solar, atmospheric, and diffuse supernovae neutrinos creates an irreducible background for direct dark matter experiments with sensitivities to WIMP-nucleon spin-independent scattering cross sections of 10-46-10-48cm2, depending on the WIMP mass. Even if one could eliminate all other backgrounds, this "neutrino floor" will limit future experiments with projected sensitivities to cross sections as small as 10-48cm2. Direction-sensitive detectors have the potential to study dark matter beyond the neutrino bound by fitting event distributions in multiple dimensions: recoil kinetic energy, recoil track angle with respect to the sun, and event time. This work quantitatively explores the impact of direction sensitivity on the neutrino bound in dark matter direct detection.The Dark Matter Time Projection Chamber 4Shooter directional dark matter detector: Calibration in a surface laboratory
Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 755 (2014) 6-19
Abstract:
The 4Shooter is a prototype dark matter detector built by the Dark Matter Time Projection Chamber (DMTPC) collaboration. The aim of the collaboration is to observe dark matter with directional sensitivity by measuring the recoil directions of nuclei struck by dark matter particles. The 4Shooter is a single time projection chamber containing CFA search for astrophysical burst signals at the Sudbury Neutrino Observatory
Astroparticle Physics Elsevier 55 (2014) 1-7
Combined analysis of all three phases of solar neutrino data from the Sudbury Neutrino Observatory
Physical Review C American Physical Society (APS) 88:2 (2013) 025501
Measurement of the νe and total 8B solar neutrino fluxes with the Sudbury Neutrino Observatory phase-III data set
Physical Review C American Physical Society (APS) 87:1 (2013) 015502