20–22 de septiembre de 2023
Europe/Madrid zona horaria

Development & Characterization of a PEN-based Wavelength Shifting Reflector

20 sept 2023, 16:30
1h 15m
Colonnade room

Colonnade room

poster Light/charge readout (PMT, SiPM, WLS, electronics etc.) Poster session

Ponente

Sr. Maximilian Goldbrunner (Department of Physics, Technical University of Munich, Garching, Germany)

Descripción

Liquid argon (LAr) detectors are deployed in rare event searches such as dark matter searches, neutrino oscillation experiments, and experiments searching for neutrinoless double beta decay. These detectors rely on wavelength shifting (WLS) materials to convert argon scintillation light (at 128 nm) to visible wavelengths, enabling efficient light collection with reflectors and detection by conventional photosensors. Tetraphenyl butadiene (TPB) is commonly used as a WLS material, but its scalability for large detectors is hindered by the requirement for vacuum evaporation to achieve high light yield. To address this challenge, we present the results from a comprehensive survey of WLS reflectors based on several reflector types, including 3M™ Enhanced Specular Reflector, Tetratex®, and Tyvek®, as well as various production grades and surface finishes of commercially available Teonex® polyethylene naphthalate (PEN) films, a potential scalable alternative to TPB. For characterization, three different facilities were used: a cryogenic VUV spectrometer at TUM, LArS – a kg-scale LAr setup instrumented with a VUV-sensitive PMT at UZH, and a 2-tonne LAr setup at CERN.

Autores primarios

Sra. Gabriela R. Araujo (Physik-Institut, University of Zürich, Switzerland) Dr. Marta Babicz (Physik-Institut, University of Zürich, Switzerland) Prof. Laura Baudis (Physik-Institut, University of Zürich, Switzerland) Dr. Pin-Jung Chiu (Physik-Institut, University of Zürich, Switzerland) Sr. Sarthak Choudhary (AstroCeNT, Nicolaus Copernicus Astronomical Centre of the Polish Academy of Sciences, Warsaw, Poland) Sr. Maximilian Goldbrunner (Department of Physics, Technical University of Munich, Garching, Germany) Sr. Vikas Gupta (Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, The Netherlands) Sra. Alice Hamer (University of Edinburgh, Edinburgh EH9 3FD, United Kingdom) Sr. Maciej Kuzwa (AstroCeNT, Nicolaus Copernicus Astronomical Centre of the Polish Academy of Sciences, Warsaw, Poland) Prof. Marcin Kuźniak (AstroCeNT, Nicolaus Copernicus Astronomical Centre of the Polish Academy of Sciences, Warsaw, Poland) Sr. Andreas Leonhardt (Department of Physics, Technical University of Munich, Garching, Germany) Sra. Elisabetta Montagna (University of Bologna and INFN sezione di Bologna, Bologna, Italy) Sr. Grzegorz Nieradka (AstroCeNT, Nicolaus Copernicus Astronomical Centre of the Polish Academy of Sciences, Warsaw, Poland) Sra. Holly B. Parkinson (University of Edinburgh, Edinburgh EH9 3FD, United Kingdom) Dr. Francesco Pietropaolo (CERN, The European Organization for Nuclear Research, 1211 Meyrin, Switzerland) Prof. Tina Pollmann (Nikhef and the University of Amsterdam, Science Park, 1098XG Amsterdam, The Netherlands) Sr. Filippo Resnati (CERN, The European Organization for Nuclear Research, 1211 Meyrin, Switzerland) Prof. Stefan Schönert (Department of Physics, Technical University of Munich, Garching, Germany) Sr. Andrzej Szelc (University of Edinburgh, Edinburgh EH9 3FD, United Kingdom) Dr. Kevin Thieme (Department of Physics and Astronomy, University of Hawai’i, Honolulu, USA) Sr. Marek Walczak (AstroCeNT, Nicolaus Copernicus Astronomical Centre of the Polish Academy of Sciences, Warsaw, Poland)

Materiales de la presentación