Measurement of cosmic ray flux in the China JinPing underground laboratory

Measurement of cosmic ray flux in the China JinPing underground laboratory
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中国金瓶地下实验室宇宙射线通量测量

DOI:
10.1088/1674-1137/37/8/086001
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发表时间:
2013-05
期刊:
影响因子:
3.6
通讯作者:
Li Jian-Min
Li Jian-Min
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
Zeng Zhi;Zhu Zhong-Hua;Yue Qian;Li Yuan-Jing;Cheng Jian-Ping;Kang Ke-Jun;Chen Yun-Hua;Li Jin;Li Jian-Min

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中国金平地下实验室(CJPL)是目前世界上运行最深的地下实验室。在如此深的地下实验室中,宇宙线通量是稀有事件实验非常重要且必要的参数。建立了一个塑料闪烁体望远镜系统来测量宇宙线通量。在CJPL附近的地面实验室利用宇宙射线对望远镜系统的性能进行了研究。根据2010年11月至2011年12月在有效寿命为171天的CJPL地下实验数据,测量到CJPL宇宙线μ子通量为(2.0±0.4)×10-10/(cm 2·s)。超低的宇宙射线背景保证了CJPL暗物质实验的理想环境。
The China JinPing underground Laboratory (CJPL) is the deepest underground laboratory running in the world at present. In such a deep underground laboratory, the cosmic ray flux is a very important and necessary parameter for rare-event experiments. A plastic scintillator telescope system has been set up to measure the cosmic ray flux. The performance of the telescope system has been studied using the cosmic rays on the ground laboratory near the CJPL. Based on the underground experimental data taken from November 2010 to December 2011 in the CJPL, which has an effective live time of 171 days, the cosmic ray muon flux in the CJPL is measured to be (2.0±0.4)×10-10/(cm2 ·s). The ultra-low cosmic ray background guarantees an ideal environment for dark matter experiments at the CJPL.
DOI: --
发表时间: 1999
期刊: --
影响因子: --
作者:
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DOI: 10.1103/physrevd.80.012001
发表时间: 2009-02
期刊: Physical Review D
影响因子: 5
作者:
B. Aharmim;S. N. Ahmed;T. Andersen;A. Anthony;N. Barros;E. Beier;A. Bellerive;B. Beltrán;M. Bergevin;S. Biller;K. Boudjemline;M. Boulay;T. Burritt;B. Cai;Y. Chan;M. Chen;M. C. Chon;B. Cleveland;G. A. Cox-Mobrand;C. Currat;X. Dai;F. Dalnoki-Veress;H. Deng;J. Detwiler;P. Doe;R. Dosanjh;G. Doucas;P.-L. Drouin;F. Duncan;M. Dunford;S. Elliott;H. C. Evans;G. Ewan;J. Farine;H. Fergani;F. Fleurot;R. Ford;J. Formaggio;N. Gagnon;J. Goon;K. Graham;D. Grant;E. Guillian;S. Habib;R. Hahn;A. Hallin;E. Hallman;C. Hargrove;P. Harvey;R. Hazama;K. Heeger;W. Heintzelman;J. Heise;R. Helmer;R. J. Hemingway;R. Henning;A. Hime;C. Howard;M. Howe;M. Huang;B. Jamieson;N. Jelley;J. Klein;M. Kos;A. Krüger;C. Kraus;C. Krauss;T. Kutter;C. Kyba;R. Lange;J. Law;I. Lawson;K. Lesko;J. Leslie;I. Levine;J. Loach;S. Luoma;R. Maclellan;S. Majerus;H. Mak;J. Maneira;A. Marino;R. Martin;N. McCauley;A. McDonald;S. Mcgee;C. Mifflin;M. Miller;B. Monreal;J. Monroe;A. Noble;N. Oblath;C. Okada;H. O'Keeffe;Y. Opachich;G. O. Gann;S. Oser;R. Ott;S. Peeters;A. Poon;G. Prior;K. Rielage;B. Robertson;R. Robertson;E. Rollin;M. Schwendener;J. Secrest;S. Seibert;O. Simard;J. Simpson;D. Sinclair;P. Skensved;M. Smith;T. Sonley;T. D. Steiger;L. Stonehill;N. Tagg;G. Tesic;N. Tolich;T. Tsui;R. D. Water;B. VanDevender;C. Virtue;D. Waller;C. Waltham;H. Tseung;D. Wark;P. Watson;J. Wendland;N. West;J. Wilkerson;J. Wilson;J. Wouters;A. Wright;M. Yeh;Fajun Zhang;K. Zuber
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影响因子: 1.4
作者:
M. Robinson;V. Kudryavtsev;R. Luscher;J. Mcmillan;P. Lightfoot;N. Spooner;N. Smith;I. Liubarsky
通讯作者: M. Robinson;V. Kudryavtsev;R. Luscher;J. Mcmillan;P. Lightfoot;N. Spooner;N. Smith;I. Liubarsky
DOI: 10.1103/physrevd.55.5282
发表时间: 1996-12
期刊: Physical Review D
影响因子: 5
作者:
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通讯作者: S. Kasahara;T. S. 2. Collaboration
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发表时间: 1998-11-01
期刊: PHYSICAL REVIEW D
影响因子: 5
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