The Korean Physical Society 06130 22, Teheran-ro 7-gil, Gangnam-gu, Seoul, Republic of Korea 610 Representation : Suk Lyun HONG TEL: 02-556-4737 FAX: 02-554-1643 E-mail : webmaster@kps.or.kr Copyright(C) KPS, All rights reserved.
30 May 2022 to 4 June 2022
Virtual Seoul
Asia/Seoul timezone

SNO+ Calibration in Scintillator Phase

Not scheduled
5m
Virtual Seoul

Virtual Seoul

Poster Neutrinoless double beta decay Poster

Description

The SNO+ experiment is a multi-purpose neutrino detector located 2 km underground at SNOLAB in Vale’s Creighton Mine in Sudbury, Ontario. The centerpiece of SNO+ is a 12-m diameter acrylic vessel (AV), containing the target medium. The AV is surrounded by 7 kilotonnes of external ultrapure water shielding and about 9400 photomultiplier tubes. SNO+ is operating in three phases, defined by the target medium: water, scintillator, and scintillator loaded with tellurium.
The physics program at SNO+ includes solar neutrino measurements, antineutrino detection, supernova neutrino monitoring, and the main physics goal: neutrinoless double beta decay search. All of these physics analyses require precise measurements of the detector's optical and timing responses using known sources to establish constraints on the energy and position reconstruction within the detector.

In its water phase, SNO+ calibrated using optical and radioactive sources developed for its predecessor, the SNO experiment, and these calibrations provide external background measurements and baseline calibration constants for the detector. The radioactive sources include the $^{16}$N and AmBe sources. The tagged 6.13~MeV $\gamma$s of the $^{16}$N source provided a clean calibration sample in the energy region of interest for both the $^8$B solar neutrinos measurement and the invisible nucleon decay search during the water phase.

Currently in the scintillator phase, some of these sources have been leveraged to provide calibration information of the scintillator from outside of the AV. These calibrations allow for measurement of the internal background and validation of the external background measured in the water phase. These calibration results will be presented. New calibration deployment systems and sources are in development to allow for calibration in the scintillator inside the AV. The status of these developments will be described. The findings from both internal and external calibrations will inform the SNO+ physics analyses.

Collaboration SNO+

Primary authors

Yi-Hsuan Lin (Queen's University/SNOLAB) Dr Ryan Bayes (Laurentian University) Mr Pouya Khaghani (Laurentian University)

Presentation materials