Projected WIMP sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment

Alex Murphy, The LUX-ZEPLIN (LZ) Collaboration

Research output: Contribution to journalArticlepeer-review

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 ducial mass, LZ is projected to exclude at 90% condence level spin-independent WIMP-nucleon cross sections above 1:410􀀀48 cm2 for a 40 GeV=c2 mass WIMP. Additionally, a 5 discovery potential is projected reaching cross sections below the exclusion limits of recent experiments. For spin-dependent WIMP-neutron(-proton) scattering, a sensitivity of 2:310􀀀43 cm2 (7:110􀀀42 cm2) for a 40 GeV=c2 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 languageEnglish
Article number052002
Number of pages14
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume101
Issue number5
DOIs
Publication statusPublished - 4 Mar 2020

Keywords

  • astro-ph.IM
  • astro-ph.CO
  • hep-ex
  • physics.ins-det

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