GPU-based optical simulation of the DARWIN detector

被引：1

作者：

Althueser, L. ^{[1
]}

Antunovic, B. ^{[2
,29
]}

Aprile, E. ^{[3
]}

Bajpai, D. ^{[4
]}

Baudis, L. ^{[5
]}

Baur, D. ^{[6
]}

Baxter, A. L. ^{[7
]}

Bellagamba, L. ^{[8
,9
]}

Biondi, R. ^{[10
]}

Biondi, Y. ^{[5
]}

Bismark, A. ^{[5
]}

Brown, A. ^{[6
]}

Budnik, R. ^{[11
]}

Chauvin, A. ^{[12
]}

Colijn, A. P. ^{[13
,14
]}

Cuenca-Garcia, J. J. ^{[15
]}

D'Andrea, V ^{[10
,16
]}

Di Gangi, P. ^{[8
,9
]}

Dierle, J. ^{[6
]}

Diglio, S. ^{[17
]}

Doerenkamp, M. ^{[12
]}

Eitel, K. ^{[15
]}

Farrell, S. ^{[18
]}

Ferella, A. D. ^{[10
,16
]}

Ferrari, C. ^{[10
]}

Findley, C. ^{[4
]}

Fischer, H. ^{[6
]}

Galloway, M. ^{[5
]}

Girard, F. ^{[5
]}

Glade-Beucke, R. ^{[6
]}

Grandi, L. ^{[19
,20
]}

Guida, M. ^{[21
]}

Hansmann-Menzemer, S. ^{[12
]}

Joerg, F. ^{[21
]}

Jones, L. ^{[4
]}

Kavrigin, P. ^{[11
]}

Krauss, L. M. ^{[22
]}

von Krosigk, B. ^{[15
]}

Kuger, F. ^{[6
]}

Landsman, H. ^{[11
]}

Lang, R. F. ^{[7
]}

Li, S. ^{[7
]}

Liang, S. ^{[18
]}

Lindner, M. ^{[21
]}

Loizeau, J. ^{[17
]}

Lombardi, F. ^{[23
]}

Undagoitia, T. Marrodan ^{[21
]}

Masbou, J. ^{[17
]}

Masson, E. ^{[24
]}

Matias-Lopes, J. ^{[25
,30
]}

机构：

[1] Westfalische Wilhelms Univ Munster, Inst Kernphys, D-48149 Munster, Germany

[2] Univ Belgrade, Vinca Inst Nucl Sci, Mihajla Petrov Alasa 12-14, Belgrade, Serbia

[3] Columbia Univ, Phys Dept, New York, NY 10027 USA

[4] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA

[5] Univ Zurich, Phys Inst, CH-8057 Zurich, Switzerland

[6] Univ Freiburg, Phys Inst, D-79104 Freiburg, Germany

[7] Purdue Univ, Dept Phys & Astron, W Lafayette, IN 47907 USA

[8] Univ Bologna, Dept Phys & Astron, I-40126 Bologna, Italy

[9] INFN Bologna, I-40126 Bologna, Italy

[10] INFN Lab Nazl Gran Sasso & Gran Sasso Sci Inst, I-67100 Laquila, Italy

[11] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-7610001 Rehovot, Israel

[12] Heidelberg Univ, Phys Inst, D-69120 Heidelberg, Germany

[13] Nikhef, Sci Pk, NL-1098 XG Amsterdam, Netherlands

[14] Univ Amsterdam, Sci Pk, NL-1098 XG Amsterdam, Netherlands

[15] Karlsruhe Inst Technol KIT, Inst Astroparticle Phys IAP, D-76344 Eggenstein Leopoldshafen, Germany

[16] Univ LAquila, Dept Phys & Chem, I-67100 Laquila, Italy

[17] Univ Nantes, SUBATECH, IMT Atlantique, CNRS,IN2P3, F-44307 Nantes, France

[18] Rice Univ, Dept Phys & Astron, Houston, TX 77005 USA

[19] Univ Chicago, Dept Phys, Chicago, IL 60637 USA

[20] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[21] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany

[22] Origins Project Fdn, Phoenix, AZ 85020 USA

[23] Johannes Gutenberg Univ Mainz, Inst Phys & Exzellenzcluster PRISMA, D-55099 Mainz, Germany

[24] Univ Paris Diderot, Univ Pierre & Marie Curie, LPNHE, CNRS,IN2P3, F-75252 Paris, France

[25] Univ Coimbra, Dept Phys, LIBPhys, P-3004516 Coimbra, Portugal

[26] Univ Calif San Diego, Dept Phys, San Diego, CA 92093 USA

[27] Stockholm Univ, Oskar Klein Ctr, Dept Phys, AlbaNova, SE-10691 Stockholm, Sweden

[28] Imperial Coll London, Imperial Ctr Inference & Cosmol, Dept Phys, London SW7 2AZ, England

[29] Univ Banja Luka, Banja Luka, Bosnia & Herceg

[30] Coimbra Polytech, ISEC, Coimbra, Portugal

[31] SISSA, Data Sci Excellence Dept, Trieste, Italy

来源：

JOURNAL OF INSTRUMENTATION | 2022年 / 17卷 / 07期

基金：

欧洲研究理事会; 以色列科学基金会; 美国国家科学基金会;

关键词：

Detector modelling and simulations I (interaction of radiation with matter; interaction of photons with matter; interaction of hadrons with matter; etc); Noble liquid detectors (scintillation; ionization; double-phase); Simulation methods and programs; Time projection Chambers (TPC); LIQUID XENON; SILICON PHOTOMULTIPLIERS; RAYLEIGH-SCATTERING; REFRACTIVE-INDEX; ULTRAVIOLET; CONSTANTS; LENGTH; LIGHT;

D O I：

10.1088/1748-0221/17/07/P07018

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

Understanding propagation of scintillation light is critical for maximizing the discovery potential of next-generation liquid xenon detectors that use dual-phase time projection chamber technology. This work describes a detailed optical simulation of the DARWIN detector implemented using Chroma, a GPU-based photon tracking framework. To evaluate the framework and to explore ways of maximizing efficiency and minimizing the time of light collection, we simulate several variations of the conventional detector design. Results of these selected studies are presented. More generally, we conclude that the approach used in this work allows one to investigate alternative designs faster and in more detail than using conventional Geant4 optical simulations, making it an attractive tool to guide the development of the ultimate liquid xenon observatory.

引用

页数：28

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