• Open Access

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

Rouven Essig, Tomer Volansky, and Tien-Tien Yu
Phys. Rev. D 96, 043017 – Published 30 August 2017

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 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.

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  • Received 14 March 2017

DOI:https://doi.org/10.1103/PhysRevD.96.043017

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.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsGravitation, Cosmology & Astrophysics

Authors & Affiliations

Rouven Essig1,*, Tomer Volansky2,†, and Tien-Tien Yu1,3,‡

  • 1C.N. Yang Institute for Theoretical Physics, Stony Brook University, Stony Brook, New York 11794, USA
  • 2Raymond and Beverly Sackler School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv 69978, Israel
  • 3Theoretical Physics Department, CERN, CH-1211 Geneva 23, Switzerland

  • *rouven.essig@stonybrook.edu
  • tomerv@post.tau.ac.il
  • tien-tien.yu@cern.ch

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Issue

Vol. 96, Iss. 4 — 15 August 2017

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