PoS - Proceedings of Science
Volume 314 - The European Physical Society Conference on High Energy Physics (EPS-HEP2017) - Neutrino Phyisics (Poster Session). Scientific Secretary: Luciano Canton.
Detector energy calibration in the STEREO neutrino experiment
V. Sergeyeva*  on behalf of the STEREO Collaboration
Full text: pdf
Pre-published on: February 21, 2018
Published on: March 20, 2018
Abstract
The STEREO experiment was developed to investigate the hypothesis of a light sterile neutrino
arising from the observed discrepancy between measured reactor antineutrino fluxes and revised
flux predictions, known as the Reactor Antineutrino Anomaly.
The detector is located at 10 m from the compact nuclear reactor core of the Institut Laue-
Langevin. The segmentation of the detector target in 6 cells allows measuring the neutrino energy
spectrum at different baselines. Antineutrino interactions are detected by the inverse beta-decay
reaction in Gd-loaded liquid scintillator.
STEREO started taking data in November 2016. About 70 days of data have been recorded during
reactor operation and 25 days during reactor shut down. STEREO plans to record 150 days
more in 2018.
To perform a correct energy reconstruction of neutrino events, the detector energy response must
be determined accurately. Different radioactive gamma-ray sources, from 0,5 to 4,4 MeV, are
used to constrain the non-linearity of the scintillator response. Calibration data analysis provides
the relation between the charge detected by the photomultipliers and the true deposited gamma
energy obtained by simulations. The main goal is to reconstruct the energy scale within a 2%
uncertainty.
DOI: https://doi.org/10.22323/1.314.0644
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