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Data-driven modeling of electron recoil nucleation in PICO C3F8 bubble chambers

Authors :
Mala Das
T. Nania
E. Behnke
L. Klopfenstein
S. Fallows
D. Tiwari
A. Plante
W. H. Lippincott
C. E. Dahl
A. Hagen
D. M. Asner
S. Sahoo
Jie Zhang
C. Licciardi
C. B. Coutu
B. Loer
M. Ardid
D. Baxter
C. B. Krauss
J. Fuentes
S. Pal
C. M. Jackson
F. Tardif
Ilan Levine
N. A. Cruz-Venegas
J. I. Collar
Satyajit Seth
Shashank Priya
K. Wierman
A. Leblanc
G. Cao
U. Chowdhury
F. Mamedov
T. Sullivan
R. Neilson
M.-C. Piro
N. Walkowski
W. Woodley
P. S. Cooper
R. Filgas
E. Weima
Amber M. Ortega
G. Crowder
O. Harris
C. Amole
T. Kozynets
S. Chen
G. Giroux
E. Vázquez-Jáuregui
P. Mitra
M. Jin
J. M. Wagner
P. Oedekerk
N. Starinski
A. Sonnenschein
B. Broerman
C. Cowles
O. Scallon
B. Hackett
A. E. Robinson
M. B. Crisler
I. J. Arnquist
F. Girard
U. Wichoski
T. Hillier
Yongke Yan
I. Stekl
Chujie Chen
C. Hardy
M. Bressler
C. D. Moore
J. Hall
J. Farine
Karl J. Clark
I. Lawson
A. J. Noble
M. Laurin
V. Zacek
Eric W. Hoppe
Source :
Physical Review D. 100
Publication Year :
2019
Publisher :
American Physical Society (APS), 2019.

Abstract

The PICO Collaboration wishes to thank SNOLAB and its staff for support through underground space, logistical and technical services. SNOLAB operations are supported by the Canada Foundation for Innovation and the Province of Ontario Ministry of Research and Innovation, with underground access provided by Vale at the Creighton mine site. We wish to acknowledge the support of the Natural Sciences and Engineering Research Council of Canada (NSERC) and the Canada Foundation for Innovation (CFI) for funding. We acknowledge the support from National Science Foundation (NSF) (Grants No. 0919526, No. 1506337, No. 1242637, No. 1205987, and No. 1806722). We acknowledge that this work is supported by the U.S. Department of Energy (DOE) Office of Science, Office of High Energy Physics (under Award No. DE-SC-0012161), by DGAPA-UNAM (PAPIIT No. IA100118) and Consejo Nacional de Ciencia y Tecnologia (CONACyT, M?exico, Grants No. 252167 and No. A1-S-8960), by the Department of Atomic Energy (DAE), Government of India, under the Centre for AstroParticle Physics II project (CAPP-II) at the Saha Institute of Nuclear Physics (SINP), European Regional Development Fund?Project ?Engineering Applications of Microworld Physics? (Project No. CZ.02.1.01/0.0/0.0/ 16_019/0000766), and the Spanish Ministerio de Ciencia, Innovacion y Universidades (Red Consolider MultiDark, Grant No. FPA2017-90566-REDC). This work is partially supported by the Kavli Institute for Cosmological Physics at the University of Chicago through NSF Grant No. 1125897, and an endowment from the Kavli Foundation and its founder Fred Kavli. We also wish to acknowledge the support from Fermi National Accelerator Laboratory under Contract No. DE-AC02-07CH11359, and Pacific Northwest National Laboratory, which is operated by Battelle for the U.S. Department of Energy under Contract No. DE-AC05- 76RL01830. We also thank Compute Canada [75] and the Center for Advanced Computing, ACENET, Calcul Qu?ebec, Compute Ontario, and WestGrid for computational support.

Details

ISSN :
24700029 and 24700010
Volume :
100
Database :
OpenAIRE
Journal :
Physical Review D
Accession number :
edsair.doi...........41d5d9d92816a9821b6285a1f36585fa
Full Text :
https://doi.org/10.1103/physrevd.100.082006