21–23 Sept 2022
University of Warsaw Library
Europe/Warsaw timezone

3DΠ scanner, an application in medical physics of the DarkSide collaboration

22 Sept 2022, 14:45
15m
316A (University of Warsaw Library)

316A

University of Warsaw Library

ul. Dobra 56/66, 00-312 Warszawa‎
Presentation Applications (dark matter, neutrino, medical physics etc.) Applications

Speaker

Azam Zabihi (Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, ASTROCENT, Warsaw, Poland)

Description

This project is based on the emerging technology from the field of direct dark matter searches for weakly interacting massive particles (WIMPs), in which Liquid Argon (LAr) time projection chambers are used to identify different particle interactions for WIMP detection. The Darkside Collaboration has demonstrated the true power of the advancing LAr detector technology. They are also making significant strides in low-radioactivity argon procurement and cryogenic photosensor development and fabrication. With these advances in hand, the principle of 3DΠ has been developed. It is a novel design of a Time Of Flight (TOF) Total-Body (TB) scanner for Positron Emission Tomography (PET) using Xenon-doped liquid Argon (LAr) as a scintillator. By doping the LAr with Xenon, the long-lifetime component of the LAr scintillation light can be suppressed, allowing the scanner to handle higher data rates and hence higher patient doses if required for a given application. Since the de-excitation process in the mixture can be accomplished with direct energy transfer from argon excimers to xenon and direct emission of xenon light, it will be faster than the fluorescence processes of a wavelength shifter (WLS). Additionally, it has been shown that reducing the operating temperature of SiPMs down to the temperature of LAr significantly reduces the dark count rate within the SiPM.
The preliminary results of the Monte Carlo simulation demonstrate that the scanner’s system performance, according to the NEMA NU 2-2018 standardized guide, is comparable to commercial scanners.

Primary author

Azam Zabihi (Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, ASTROCENT, Warsaw, Poland)

Co-authors

Prof. Andrew Renshaw (University of Houston, Department of Physics, Hoston, United States of America) Dr Masayuki Wada (Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, ASTROCENT, Warsaw, Poland) Mr Alejandro Ramirez (University of Houston, Department of Physics, Hoston, United States of America) Dr Michela Lai (University of Cagliari, Department of Physics, Cagliari, Italy) Dr Federico Gabriele (INFN Cagliari Division, INFN, Cagliari, Italy) Dr Xinran Li (Lawrence Berkeley National Laboratory, Berkeley, CA 94720, United States of America) Prof. Cristian Galbiati (Gran Sasso Science Institute, L’Aquila 67100, Italy-Princeton University, Department of Physics, Princeton, United States of America) Prof. Davide Franco (APC, University of Paris, CNRS, Astroparticle and Cosmology, Paris F- 75013, France)

Presentation materials