Abstract
LUX-ZEPLIN (LZ) is a next generation dark matter direct detection
experiment that will operate 4850 feet underground at the Sanford
Underground Research Facility (SURF) in Lead, South Dakota, USA. Using a
two-phase xenon detector with an active mass of 7 tonnes, LZ will
search primarily for low-energy interactions with Weakly Interacting
Massive Particles (WIMPs), which are hypothesized to make up the dark
matter in our galactic halo. In this paper, the projected WIMP
sensitivity of LZ is presented based on the latest background estimates
and simulations of the detector. For a 1000 live day run using a 5.6
tonne fiducial mass, LZ is projected to exclude at 90% confidence level
spin-independent WIMP-nucleon cross sections above $1.6 \times 10^{-48}$
cm$^{2}$ for a 40 $\mathrm{GeV}/c^{2}$ mass WIMP. Additionally, a
$5\sigma$ discovery potential is projected reaching cross sections below
the existing and projected exclusion limits of similar experiments that
are currently operating. For spin-dependent WIMP-neutron(-proton)
scattering, a sensitivity of $2.7 \times 10^{-43}$ cm$^{2}$ ($8.1 \times
10^{-42}$ cm$^{2}$) for a 40 $\mathrm{GeV}/c^{2}$ mass WIMP is
expected. With construction well underway, LZ is on track for
underground installation at SURF in 2019 and will start collecting data
in 2020.
Original language | English |
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Article number | 052002 |
Number of pages | 17 |
Journal | Physical Review D |
Volume | 101 |
Issue number | 5 |
DOIs | |
Publication status | Published - 4 Mar 2020 |
Keywords
- astro-ph.IM
- astro-ph.CO
- hep-ex
- physics.ins-det