Enectali Figueroa-Feliciano
Readout strategies for directional dark matter detection beyond the neutrino background
Figueroa-Feliciano, Enectali; O'Hare, Ciaran A.J.; Green, Anne M.; Billard, Julien; Strigari, Louis E.
Authors
Ciaran A.J. O'Hare
Professor ANNE GREEN anne.green@nottingham.ac.uk
PROFESSOR OF PHYSICS
Julien Billard
Louis E. Strigari
Abstract
© 2015 American Physical Society. The search for weakly interacting massive particles (WIMPs) by direct detection faces an encroaching background due to coherent neutrino-nucleus scattering. As the sensitivity of these experiments improves, the question of how to best distinguish a dark matter signal from neutrinos will become increasingly important. A proposed method of overcoming this so-called "neutrino floor" is to utilize the directional signature that both neutrino- and dark-matter-induced recoils possess. We show that directional experiments can indeed probe WIMP-nucleon cross sections below the neutrino floor with little loss in sensitivity due to the neutrino background. In particular we find at low WIMP masses (around 6 GeV) the discovery limits for directional detectors penetrate below the nondirectional limit by several orders of magnitude. For high WIMP masses (around 100 GeV), the nondirectional limit is overcome by a factor of a few. Furthermore we show that even for directional detectors which can only measure one- or two-dimensional projections of the three-dimensional recoil track, the discovery potential is only reduced by a factor of 3 at most. We also demonstrate that while the experimental limitations of directional detectors, such as sense recognition and finite angular resolution, have a detrimental effect on the discovery limits, it is still possible to overcome the ultimate neutrino background faced by nondirectional detectors.
Citation
Figueroa-Feliciano, E., O'Hare, C. A., Green, A. M., Billard, J., & Strigari, L. E. (2015). Readout strategies for directional dark matter detection beyond the neutrino background. Physical Review D - Particles, Fields, Gravitation and Cosmology, 92(6), https://doi.org/10.1103/PhysRevD.92.063518
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 1, 2015 |
Online Publication Date | Sep 17, 2015 |
Publication Date | Sep 17, 2015 |
Deposit Date | Jun 30, 2016 |
Publicly Available Date | Jun 30, 2016 |
Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
Print ISSN | 1550-7998 |
Electronic ISSN | 1550-2368 |
Publisher | American Physical Society |
Peer Reviewed | Peer Reviewed |
Volume | 92 |
Issue | 6 |
DOI | https://doi.org/10.1103/PhysRevD.92.063518 |
Public URL | https://nottingham-repository.worktribe.com/output/761004 |
Publisher URL | http://journals.aps.org/prd/abstract/10.1103/PhysRevD.92.063518 |
Related Public URLs | http://journals.aps.org/prd/abstract/10.1103/PhysRevD.92.063518 |
Contract Date | Jun 30, 2016 |
Files
1505.08061.pdf
(983 Kb)
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