2015
DOI: 10.1103/physrevd.92.083517
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Modulation effects in dark matter-electron scattering experiments

Abstract: One of the next frontiers in dark-matter direct-detection experiments is to explore the MeV to GeV mass regime. Such light dark matter does not carry enough kinetic energy to produce an observable nuclear recoil, but it can scatter off electrons, leading to a measurable signal. We introduce a semi-analytic approach to characterize the resulting electron-scattering events in atomic and semiconductor targets, improving on previous analytic proposals that underestimate the signal at high recoil energies. We then … Show more

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Cited by 158 publications
(201 citation statements)
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References 68 publications
(120 reference statements)
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“…One irreducible background is from neutrino-electron scattering, which sets the ultimate limit to the sub-GeV DM direct detections. Fortunately, the DM annual modulation effect from the motion of the earth can be employed to reduce the neutrino background [39,41,42]. The teens MeV DM of concern could be probed via the inelastic processes of DM-electron scatterings, e.g.…”
Section: Dm-electron Scatteringmentioning
confidence: 99%
“…One irreducible background is from neutrino-electron scattering, which sets the ultimate limit to the sub-GeV DM direct detections. Fortunately, the DM annual modulation effect from the motion of the earth can be employed to reduce the neutrino background [39,41,42]. The teens MeV DM of concern could be probed via the inelastic processes of DM-electron scatterings, e.g.…”
Section: Dm-electron Scatteringmentioning
confidence: 99%
“…Current direct-detection bounds from XENON10 [28] are not yet sensitive to in the range predicted by the ELDER scenario, while the collider bounds from LEP-2 depend strongly on the mass of the particle mediating the DM-SM scattering, and cannot be used to put robust constrains on . Interestingly, proposed dedicated germanium or silicon-based electron-recoil direct detection experiments [29,30] and superconducting detectors [31] are expected to directly probe the ELDER scenario, which gives a scattering cross-section with electrons, σ scat ∼ 10 −40 − 10 −41 cm 2 . Finally, the strong 3 → 2 self-annihilations required in the ELDER scenario generically imply a large contribution to χχ → χχ elastic self-scattering.…”
Section: Constraintsmentioning
confidence: 99%
“…The process of dark matter-electron scattering is derived and discussed in references [9][10][11][12]. In this section we summarise the key findings of [10], which are necessary to discuss the expected sensitivity for RNDR DEPFET dark matter detectors in Sect.…”
Section: Detection Of Mev Dark Matter By Dark Matter-electron Scatteringmentioning
confidence: 99%
“…This topic has been discussed in detail in the literature, e.g. in [9][10][11][12], and is only summarised here.…”
Section: Introductionmentioning
confidence: 99%