Abstract

The Accelerator Neutrino Neutron Interaction Experiment (ANNIE) aims to make a unique measurement of neutron yield from neutrino-nucleus interactions and to perform R&D for the next generation of water-based neutrino detectors. In this paper, we characterize beam-induced neutron backgrounds in the experimental hall at Fermi National Accelerator Laboratory. It is shown that the background levels are sufficiently low to allow the next stage of the experiment to proceed. These measurements are relevant to other Booster Neutrino Beam (BNB) [1] experiments located adjacent to ANNIE Hall, where dirt neutrons and sky-shine could present similar backgrounds.

Highlights

  • The Accelerator Neutrino Neutron Interaction Experiment (ANNIE) [2] aims to make the first detailed measurement of the number of neutrons produced by muon neutrinos interacting with nuclei

  • Because the algorithms used to reconstruct the photomultiplier tubes (PMTs) pulses rely on a threshold based on pulse amplitude rather than charge, the total charge collected by the two Neutron Capture Volume (NCV) PMTs for events at threshold should be distributed about some mean value (Qthresh)

  • Assuming that the total charge measured by the NCV PMTs is approximately a linear function of the energy deposited in the liquid scintillator, the NCV energy threshold Ethresh may be written in the form

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Summary

Introduction

The Accelerator Neutrino Neutron Interaction Experiment (ANNIE) [2] aims to make the first detailed measurement of the number of neutrons produced by muon neutrinos interacting with nuclei. At concentrations of 0.1% Gd by mass, the enhanced cross-section has the added benefit of shortening the time constant for neutron capture from ∼200 μs to ∼30 μs These combined effects make Gd-loading essential to the final-state neutron multiplicity measurement. We report a first measurement of beam-correlated background neutrons in the ANNIE tank as a function of position This analysis uses data taken in a special configuration (ANNIE Phase-I) of the detector with a pure water target. We use the measured fall-off as a function of distance from the surface of the water and the tank walls in Phase-I to verify that that the proposed buffer region surrounding the optically isolated volume for the main ANNIE neutrino interaction physics program, known as Phase-II (lower panel of figure 1), provides adequate shielding from background neutrons. The techniques described in this paper will be applicable to any future water-based near detectors, especially those with Gd-loading or water-based liquid scintillators

Experimental design of the neutron background measurement
Upstream and downstream veto and muon selection
Data taking and selection
Signal processing
Pedestal estimation
Pulse finding
Waveform calibration
Feature extraction
Neutron candidate selection
NCV coincidence requirement
After-pulsing requirement
Total charge cut
Water PMT veto cut
Arrival time distribution of detected neutrons from a 252Cf source
NCV energy threshold measurement using cosmic muon data
Charge threshold measurement
Peak charge measurement
Calculation of the energy threshold
Estimation of the NCV efficiency
Estimating the NCV efficiency using the energy threshold
Computing the beam-induced neutron event count
CIT background estimation using pre-beam data
CIT background estimation using late-time data
After-pulsing correction
Beam-correlated neutron event counts
10.1 Systematic uncertainties on Nn
10.2 Measurement of NCV and associated systematic error
10.3 Systematic uncertainties in exposure and volume scaling
10.4 Combined uncertainty estimate
11 Implications for the ANNIE neutron multiplicity measurement
Findings
12 Conclusions

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