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E

E. Reid

Researcher at Durham University

Publications -  14
Citations -  495

E. Reid is an academic researcher from Durham University. The author has contributed to research in topics: Neutrino & Dark matter. The author has an hindex of 6, co-authored 8 publications receiving 247 citations.

Papers
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Journal ArticleDOI

Constraints on low-mass, relic dark matter candidates from a surface-operated SuperCDMS single-charge sensitive detector

D. W. P. Amaral, +128 more
- 28 May 2020 - 
TL;DR: In this article, the authors present an analysis and the resulting limits on light dark matter inelastically scattering off of electrons, and on dark photon and axion-like particle absorption, using a second-generation SuperCDMS high-voltage eV-resolution detector.
Journal ArticleDOI

How high is the neutrino floor

TL;DR: In this article, the contribution of neutrino-nucleus scattering cross-sections to the coherent elastic neutrinos scattering cross section from new physics models in the neutrini sector is computed.
Journal ArticleDOI

Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated above Ground.

I. Alkhatib, +135 more
TL;DR: This exclusion analysis sets the most stringent dark matter-nucleon scattering cross-section limits achieved by a cryogenic detector for dark matter particle masses from 93 to 140 MeV/c^{2}, with a raw exposure of 9.9 g d acquired at an above-ground facility.
Journal ArticleDOI

How high is the neutrino floor

TL;DR: In this paper, the contribution to the coherent elastic neutrino-nucleus scattering cross-section from new physics models in the Neutrino sector has been calculated.
Journal ArticleDOI

Solar neutrino probes of the muon anomalous magnetic moment in the gauged U 1 L μ − L τ $$ \mathrm{U}{(1)}_{L_{\mu }-{L}_{\tau }} $$

TL;DR: In this paper, the authors reevaluate Borexino constraints on neutrino-electron scattering, finding them to be more stringent than previously reported, and already excluding a part of the (g − 2)μ explanation with mediator masses smaller than 2 × 10−2 GeV.