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5–11 Jun 2022
McMaster University
America/Toronto timezone
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(G*) (POS-33) Optical Calibration of the SNO+ Detector using Internal Backgrounds

7 Jun 2022, 17:42
2m
MUSC Marketplace (McMaster University)

MUSC Marketplace

McMaster University

Poster Competition (Graduate Student) / Compétition affiches (Étudiant(e) 2e ou 3e cycle) Particle Physics / Physique des particules (PPD) PPD Poster Session & Student Poster Competition (21) | Session d'affiches PPD et concours d'affiches étudiantes (21)

Speakers

Dr Serena Riccetto (Queen's University)Ms Rayhaneh Dehghani (Queen's University) Anthony Allega (Queen's University)

Description

The SNO+ experiment is a multipurpose neutrino detector located 2 km underground at SNOLAB in Sudbury, Ontario. The primary goal of the experiment is to search for neutrinoless double beta $(0\nu\beta\beta)$ decay in liquid scintillator loaded with $^{130}$Te in a low-background environment. An observation of a $0\nu\beta\beta$ decay signal would demonstrate the Majorana nature of neutrinos. In order to resolve such a rare decay process, a precise optical calibration of the SNO+ detector is critical. This work presents a sensitive method of investigating the attenuation parameters in liquid scintillator by modelling the simulated radial light yield profiles of various internal background sources. The scintillator materials utilized in the SNO+ Monte Carlo (MC) simulation framework have been fine-tuned based on ex-situ measurements of the light yield and comparison to detector data.

Primary author

Dr Serena Riccetto (Queen's University)

Co-authors

Ms Rayhaneh Dehghani (Queen's University) Anthony Allega (Queen's University)

Presentation materials