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Title: New constraints and prospects for sub-GeV dark matter scattering off electrons in xenon

Abstract

We study in detail sub-GeV dark matter scattering off electrons in xenon, including the expected electron recoil spectra and annual modulation spectra. We derive improved constraints using low-energy XENON10 and XENON100 ionization-only data. For XENON10, in addition to including electron-recoil data corresponding to about 1–3 electrons, we include for the first time events corresponding to about 4–7 electrons. Assuming the scattering is momentum independent (FDM = 1 ), this strengthens a previous cross-section bound by almost an order of magnitude for dark matter masses above 50 MeV. The available XENON100 data corresponds to events with about 4–50 electrons, and leads to a constraint that is comparable to the XENON10 bound above 50 MeV for FDM = 1 . We demonstrate that a search for an annual modulation signal in upcoming xenon experiments (XENON1T, XENONnT, LZ) could substantially improve the above bounds even in the presence of large backgrounds. We also emphasize that in simple benchmark models of sub-GeV dark matter, the dark matter-electron scattering rate can be as high as one event every ten (two) seconds in the XENON1T (XENONnT or LZ) experiments, without being in conflict with any other known experimental bounds. While there are several sources of backgroundsmore » that can produce single- or few-electron events, a large event rate can be consistent with a dark matter signal and should not be simply written off as purely a detector curiosity. This fact motivates a detailed analysis of the ionization-data (“S2”) data, taking into account the expected annual modulation spectrum of the signal rate, as well as the DM-induced electron-recoil spectra, which are another powerful discriminant between signal and background.« less

Authors:
; ;
Publication Date:
Research Org.:
New York Univ. (NYU), NY (United States)
Sponsoring Org.:
USDOE
OSTI Identifier:
1377658
Alternate Identifier(s):
OSTI ID: 1426144
Grant/Contract Number:  
SC0008061
Resource Type:
Published Article
Journal Name:
Physical Review D
Additional Journal Information:
Journal Name: Physical Review D Journal Volume: 96 Journal Issue: 4; Journal ID: ISSN 2470-0010
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS

Citation Formats

Essig, Rouven, Volansky, Tomer, and Yu, Tien-Tien. New constraints and prospects for sub-GeV dark matter scattering off electrons in xenon. United States: N. p., 2017. Web. doi:10.1103/PhysRevD.96.043017.
Essig, Rouven, Volansky, Tomer, & Yu, Tien-Tien. New constraints and prospects for sub-GeV dark matter scattering off electrons in xenon. United States. doi:10.1103/PhysRevD.96.043017.
Essig, Rouven, Volansky, Tomer, and Yu, Tien-Tien. Wed . "New constraints and prospects for sub-GeV dark matter scattering off electrons in xenon". United States. doi:10.1103/PhysRevD.96.043017.
@article{osti_1377658,
title = {New constraints and prospects for sub-GeV dark matter scattering off electrons in xenon},
author = {Essig, Rouven and Volansky, Tomer and Yu, Tien-Tien},
abstractNote = {We study in detail sub-GeV dark matter scattering off electrons in xenon, including the expected electron recoil spectra and annual modulation spectra. We derive improved constraints using low-energy XENON10 and XENON100 ionization-only data. For XENON10, in addition to including electron-recoil data corresponding to about 1–3 electrons, we include for the first time events corresponding to about 4–7 electrons. Assuming the scattering is momentum independent (FDM = 1 ), this strengthens a previous cross-section bound by almost an order of magnitude for dark matter masses above 50 MeV. The available XENON100 data corresponds to events with about 4–50 electrons, and leads to a constraint that is comparable to the XENON10 bound above 50 MeV for FDM = 1 . We demonstrate that a search for an annual modulation signal in upcoming xenon experiments (XENON1T, XENONnT, LZ) could substantially improve the above bounds even in the presence of large backgrounds. We also emphasize that in simple benchmark models of sub-GeV dark matter, the dark matter-electron scattering rate can be as high as one event every ten (two) seconds in the XENON1T (XENONnT or LZ) experiments, without being in conflict with any other known experimental bounds. While there are several sources of backgrounds that can produce single- or few-electron events, a large event rate can be consistent with a dark matter signal and should not be simply written off as purely a detector curiosity. This fact motivates a detailed analysis of the ionization-data (“S2”) data, taking into account the expected annual modulation spectrum of the signal rate, as well as the DM-induced electron-recoil spectra, which are another powerful discriminant between signal and background.},
doi = {10.1103/PhysRevD.96.043017},
journal = {Physical Review D},
number = 4,
volume = 96,
place = {United States},
year = {2017},
month = {8}
}

Journal Article:
Free Publicly Available Full Text
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DOI: 10.1103/PhysRevD.96.043017

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