Projected sensitivities of the LUX-ZEPLIN experiment to new physics via low-energy electron recoils
File(s) PhysRevD.104.092009.pdf (1.73 MB)
Published version
Author(s)
Type
Journal Article
Abstract
LUX-ZEPLIN is a dark matter detector expected to obtain world-leading sensitivity to weakly-interacting massive particles interacting via nuclear recoils with a
∼
7
-tonne xenon target mass. This paper presents sensitivity projections to several low-energy signals of the complementary electron recoil signal type: 1) an effective neutrino magnetic moment, and 2) an effective neutrino millicharge, both for
p
p
-chain solar neutrinos, 3) an axion flux generated by the Sun, 4) axionlike particles forming the Galactic dark matter, 5) hidden photons, 6) mirror dark matter, and 7) leptophilic dark matter. World-leading sensitivities are expected in each case, a result of the large 5.6 t 1000 d exposure and low expected rate of electron-recoil backgrounds in the
<
100
keV
energy regime. A consistent signal generation, background model and profile-likelihood analysis framework is used throughout.
∼
7
-tonne xenon target mass. This paper presents sensitivity projections to several low-energy signals of the complementary electron recoil signal type: 1) an effective neutrino magnetic moment, and 2) an effective neutrino millicharge, both for
p
p
-chain solar neutrinos, 3) an axion flux generated by the Sun, 4) axionlike particles forming the Galactic dark matter, 5) hidden photons, 6) mirror dark matter, and 7) leptophilic dark matter. World-leading sensitivities are expected in each case, a result of the large 5.6 t 1000 d exposure and low expected rate of electron-recoil backgrounds in the
<
100
keV
energy regime. A consistent signal generation, background model and profile-likelihood analysis framework is used throughout.
Date Issued
2021-11-23
Date Acceptance
2021-09-22
Citation
Physical Review D: Particles, Fields, Gravitation and Cosmology, 2021, 104 (9), pp.1-16
ISSN
1550-2368
Publisher
American Physical Society
Start Page
1
End Page
16
Journal / Book Title
Physical Review D: Particles, Fields, Gravitation and Cosmology
Volume
104
Issue
9
Copyright Statement
© 2021 The Author(s). Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
License URL
Identifier
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000723098900006&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
Subjects
Science & Technology
Physical Sciences
Astronomy & Astrophysics
Physics, Particles & Fields
Physics
DARK-MATTER
SOLAR AXIONS
SEARCH
NEUTRINO
LIMITS
XMASS
MODEL
Publication Status
Published
Article Number
ARTN 092009
Date Publish Online
2021-11-23
