Projected WIMP sensitivity of the LUX-ZEPLIN dark matter experiment
File(s)1802.06039v2.pdf (2.3 MB)
Accepted version
Author(s)
Type
Journal Article
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
1.4
×
10
−
48
cm
2
for a
40
GeV
/
c
2
mass WIMP. Additionally, a
5
σ
discovery potential is projected, reaching cross sections below the exclusion limits of recent experiments. For spin-dependent WIMP-neutron(-proton) scattering, a sensitivity of
2.3
×
10
−
43
cm
2
(
7.1
×
10
−
42
cm
2
) for a
40
GeV
/
c
2
mass WIMP is expected. With underground installation well underway, LZ is on track for commissioning at SURF in 2020.
1.4
×
10
−
48
cm
2
for a
40
GeV
/
c
2
mass WIMP. Additionally, a
5
σ
discovery potential is projected, reaching cross sections below the exclusion limits of recent experiments. For spin-dependent WIMP-neutron(-proton) scattering, a sensitivity of
2.3
×
10
−
43
cm
2
(
7.1
×
10
−
42
cm
2
) for a
40
GeV
/
c
2
mass WIMP is expected. With underground installation well underway, LZ is on track for commissioning at SURF in 2020.
Date Issued
2020-03-04
Date Acceptance
2019-12-02
Citation
Physical Review D: Particles, Fields, Gravitation and Cosmology, 2020, 101 (5), pp.1-17
ISSN
1550-2368
Publisher
American Physical Society
Start Page
1
End Page
17
Journal / Book Title
Physical Review D: Particles, Fields, Gravitation and Cosmology
Volume
101
Issue
5
Copyright Statement
© 2020 American Physical Society.
Sponsor
Science and Technology Facilities Council (STFC)
Identifier
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000517963200002&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
Grant Number
ST/P00377X/1
Subjects
Science & Technology
Physical Sciences
Astronomy & Astrophysics
Physics, Particles & Fields
Physics
LOADED LIQUID SCINTILLATOR
XENON
SIMULATION
LIMITS
RADIOACTIVITY
BACKGROUNDS
EMISSION
DETECTOR
RECOIL
GASES
Publication Status
Published
Article Number
ARTN 052002
Date Publish Online
2020-03-04