Abstract

Coherent elastic neutrino–nucleus scattering (hbox {CE}nu hbox {NS}) offers a unique way to study neutrino properties and to search for new physics beyond the Standard Model. Nuclear reactors are promising sources to explore this process at low energies since they deliver large fluxes of anti-neutrinos with typical energies of a few MeV. In this paper, a new-generation experiment to study hbox {CE}nu hbox {NS} is described. The NUCLEUS experiment will use cryogenic detectors which feature an unprecedentedly low-energy threshold and a time response fast enough to be operated under above-ground conditions. Both sensitivity to low-energy nuclear recoils and a high event rate tolerance are stringent requirements to measuring hbox {CE}nu hbox {NS} of reactor anti-neutrinos. A new experimental site, the Very-Near-Site (VNS), at the Chooz nuclear power plant in France is described. The VNS is located between the two 4.25 hbox {GW}_{mathrm {th}} reactor cores and matches the requirements of NUCLEUS. First results of on-site measurements of neutron and muon backgrounds, the expected dominant background contributions, are given. In this paper a preliminary experimental set-up with dedicated active and passive background reduction techniques and first background estimations are presented. Furthermore, the feasibility to operate the detectors in coincidence with an active muon veto at shallow overburden is studied. The paper concludes with a sensitivity study pointing out the physics potential of NUCLEUS at the Chooz nuclear power plant.

Highlights

  • The existence of neutral-current neutrino interactions implies the existence of elastic neutrino–nucleus scattering [1]

  • This paper describes the NUCLEUS experiment at the Chooz Very-Near-Site (VNS), designed to study CEνNS using reactor anti-neutrinos

  • The site is located in close distance to the two 4.25 GWth reactor cores of the Chooz nuclear power plant in France, providing an anti-neutrino flux of 3 × 1012 ν/(s · cm2)

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Summary

Introduction

The existence of neutral-current neutrino interactions implies the existence of elastic neutrino–nucleus scattering [1]. Contrary to the enhancement of the cross-section, the experimental signature, i.e. the nuclear recoil, is suppressed in energy by the nucleus mass, mN. The enhancement of the CEνNS cross-section allows for a miniaturization of neutrino detectors, from the typical tonne-size to kilogram- or even gramscale in the case of NUCLEUS, and a possible practical application in nuclear reactor monitoring [13]. CEνNS of solar and atmospheric neutrinos will become an irreducible background for future dark matter experiments searching for weakly interacting massive particles, which profit from an independent measurement of the cross-section. This paper describes the NUCLEUS experiment at the Chooz Very-Near-Site (VNS), designed to study CEνNS using reactor anti-neutrinos.

The Very-Near-Site at the Chooz nuclear power plant
Description of the VNS
Measurement of the muon flux attenuation
Measurement of the fast neutron flux reduction
The NUCLEUS experiment at the VNS
Sources of background
The NUCLEUS target detectors
The cryostat
Active and passive shielding
The BASKET detectors
Muon-induced dead time considerations
Monte Carlo simulations of cosmic muons at the VNS
Estimation of muon-induced dead time
Background studies
Atmospheric neutrons
Muon-induced neutrons
External γ -rays
Surface events
Intrinsic background of CaWO4 crystals
Cosmogenic activation of CaWO4 crystals
Reactor-correlated neutrons
Sensitivity of NUCLEUS-10g for different flat backgrounds
Sensitivity of NUCLEUS to CEνNS at the VNS
Achievable precision of NUCLEUS-10g and -1kg
NUCLEUS-10g in the case of a non-flat background
Findings
Conclusion
Full Text
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