Data-driven modeling of electron recoil nucleation in PICO C3F8 bubble chambers
Data-driven modeling of electron recoil nucleation in PICO C3F8 bubble chambers
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DOI：
10.1103/physrevd.100.082006
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发表时间：
2019-05
影响因子：
5
通讯作者：
C. Amole;M. Ardid;I. Arnquist;D. Asner;D. Baxter;E. Behnke;M. Bressler;B. Broerman;G. Cao
中科院分区：
文献类型：
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作者：
C. Amole;M. Ardid;I. Arnquist;D. Asner;D. Baxter;E. Behnke;M. Bressler;B. Broerman;G. Cao
皮科协作团队感谢SNOLAB及其员工通过地下空间、后勤和技术服务提供的支持。SNOLAB的运营得到了加拿大创新基金会和安大略省研究与创新部的支持，淡水河谷在Creighton矿场提供了地下通道。我们感谢加拿大自然科学和工程研究理事会（NSERC）和加拿大创新基金会（CFI）的资助。我们感谢国家科学基金会（NSF）的支持（赠款编号0919526、1506337、1242637、1205987和1806722）。我们承认这项工作得到了美国能源部（DOE）科学办公室、高能物理办公室（奖励编号DE-SC-0012161）、DGAPA-UNAM（PAPIIT编号IA 100118）和国家科学技术委员会（CONACyT，M？印度政府原子能部在欧洲区域发展基金萨哈核物理研究所天体粒子物理学中心二期项目下提供的技术援助（第252167号和第A1-S-8960号赠款）。项目？微观世界物理的工程应用（项目编号CZ.02.1.01/0.0/0.0/ 16_019/0000766）和西班牙城市、创新和大学部（Red Consolider MultiDark，批准号FPA 2017 -90566-REDC）。这项工作得到了芝加哥大学Kavli宇宙物理研究所通过NSF资助号1125897的部分支持，以及Kavli基金会及其创始人Fred Kavli的捐赠。我们还要感谢费米国家加速器实验室（合同号：DE-AC 02 - 07 CH 11359）和太平洋西北国家实验室（由巴特尔为美国能源部运营，合同号：DE-AC 05 - 76 RL 01830）的支持。我们还要感谢加拿大计算[75]和先进计算中心，ACENET，Calcul Qu？ebec、Compute安大略和WestGrid提供计算支持。
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.