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Measurement of scintillation response of CsI[Na] to low-energy nuclear recoils by COHERENT
Abstract
We present results of several measurements of CsI[Na] scintillation response
to 3-60 keV energy nuclear recoils performed by the COHERENT collaboration
using tagged neutron elastic scattering experiments and an endpoint technique.
Earlier results, used to estimate the coherent elastic neutrino-nucleus
scattering (CEvNS) event rate for the first observation of this process
achieved by COHERENT at the Spallation Neutron Source (SNS), have been
reassessed. We discuss corrections for the identified systematic effects and
update the respective uncertainty values. The impact of updated results on
future precision tests of CEvNS is estimated. We scrutinize potential
systematic effects that could affect each measurement. In particular we confirm
the response of the H11934-200 Hamamatsu photomultiplier tube (PMT) used for
the measurements presented in this study to be linear in the relevant signal
scale region.
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https://hdl.handle.net/10161/23986Collections
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Show full item recordScholars@Duke
Phillip S. Barbeau
Associate Professor of Physics
Professor Barbeau’s research interests are predominantly in the fields of neutrino
and astroparticle physics. His efforts are focused on (but not limited to) three major
areas of research: studying the physics of coherent neutrino-nucleus scattering; novel
searches for the dark matter in our universe; and searches for zero neutrino double
beta decay. The unifying aspect of the work is the common need for new and creative
detector development in order to solve some of the “hard”
Kate Scholberg
Arts & Sciences Distinguished Professor of Physics
Prof. Scholberg's broad research interests include experimental elementary particle
physics, astrophysics and cosmology. Her main specific interests are in neutrino physics:
she studies neutrino oscillations with the Super-Kamiokande experiment, a giant underground
water Cherenkov detector located in a mine in the Japanese Alps. Super-K was constructed
to search for proton decay and to study neutrinos from the sun, from cosmic ray collisions
in the atmosphere, and from supernovae. On Super-K, Pr
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