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arxiv: 1407.7524 · v2 · submitted 2014-07-28 · ⚛️ physics.ins-det · astro-ph.IM· hep-ex· hep-ph· nucl-ex

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Coherent neutrino-nucleus scattering detection with a CsI[Na] scintillator at the SNS spallation source

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classification ⚛️ physics.ins-det astro-ph.IMhep-exhep-phnucl-ex
keywords cennsdetectioncoherentcross-sectionlow-energyneutrinoneutrino-nucleusscattering
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We study the possibility of using CsI[Na] scintillators as an advantageous target for the detection of coherent elastic neutrino-nucleus scattering (CENNS), using the neutrino emissions from the SNS spallation source at Oak Ridge National Laboratory. The response of this material to low-energy nuclear recoils like those expected from this process is characterized. Backgrounds are studied using a 2 kg low-background prototype crystal in a dedicated radiation shield. The conclusion is that a planned 14 kg detector should measure approximately 550 CENNS events per year above a demonstrated $\sim7$ keVnr low-energy threshold, with a signal-to-background ratio sufficient for a first measurement of the CENNS cross-section. The cross-section for the $^{208}$Pb($\nu_{e},e^{-}$)$^{208}$Bi reaction, of interest for future supernova neutrino detection, can be simultaneously obtained.

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  1. Cryogenic pure CsI as a probe for neutrino electromagnetic interactions

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    Cryogenic pure CsI converts the suppression of nuclear recoil ionization into a selective probe for neutrino-electron scattering, enabling better constraints on neutrino electromagnetic couplings at reactor sites.