Bulletin of the American Physical Society
APS April Meeting 2019
Volume 64, Number 3
Saturday–Tuesday, April 13–16, 2019; Denver, Colorado
Session G17: WIMP Dark Matter I
8:30 AM–10:18 AM,
Sunday, April 14, 2019
Sheraton
Room: Grand Ballroom II
Sponsoring
Unit:
DPF
Chair: Bjoern Penning
Abstract: G17.00001 : Search for WIMP Dark-Matter Inelastic Interactions using a Lead Target*
8:30 AM–8:42 AM
Presenter:
Thomas E Ward
(TechSource (United States), US DOE/Techsource)
Authors:
Thomas E Ward
(TechSource (United States), US DOE/Techsource)
Alexander Androvich Rimsky-Korsakov
(Kholopin Radium Institute)
Nikolai e Kudryashev
(Kholopin Radium Institute)
Alexander e Barzilov
(University of Nevada at Las Vegas)
Denis e Beller
(University of Nevada at Las Vegas)
Jhuli e Peltoniemi
(University of Oulu)
A 270 live-day search for inelastic (indirect) scattering of WIMP dark matter with baryonic matter using a 300 kg Pb target and 64-element neutron multiplicity detector system (NMDS) at 583 m.w.e was undertaken at the CUPP underground facility in Finland. The study resulted in a detection limit of 3 neutral candidate events each producing ~140 neutrons in a single point interaction yielding a nucleon cross-section limit of <5.5E(-43)cm^-2 . The complete disintegration of the Pb nucleus in a central weak interaction annihilation with WIMP DM is the key signature of the indirect inelastic event. The equivalent direct (elastic) cross-section limit of <7.6E(-45)cm^-2 , based on the Compton wavelength of 8 GeV DM, is near the current detection limit for massive recoil detectors (LUX, XENON1T, PandaX-II, 2017). NMDS events induced by muons in the target were found to be within +/-15% agreement with measurements and predictions of previous underground studies at CUPP (2005) and Mei and Hime (2006) at several underground laboratories.
*This work was supported in part by US DOE-Office of Nuclear Energy Contract Number DE-DT0004091
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