Simulation of the cosmic ray tau neutrino telescope (CRTNT) experiment
Liu JL(刘加丽); Zhang SS(张寿山); Cao Z(曹臻); He HH(何会海); Xiao G(肖刚); Cha M(查敏); Zhang BK(张丙开); Bai YX(白云翔); Zhang Y(张勇); Liu, JL; Zhang, SS; Cao, Z; He, HH; Huang, MA; Liu, TC; Xiao, G; Zha, M; Zhang, BK; Bai, YX; Zhang, Y
刊名JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS
2009
卷号36期号:7页码:75201
学科分类Physics
DOI10.1088/0954-3899/36/7/075201
通讯作者[Liu, J. L. ; Zhang, S. S. ; Cao, Z. ; He, H. H. ; Xiao, G. ; Zha, M. ; Zhang, B. K. ; Bai, Y. X. ; Zhang, Y.] Inst High Energy Phys, Key Lab Astroparticle Phys, Beijing 100049, Peoples R China ; [Huang, M. A.] Natl United Univ, Dept Energy & Resources, Miaoli 36003, Taiwan ; [Liu, T. C.] Natl Chiao Tung Univ, Inst Phys, Hsinchu 300, Taiwan
文章类型Article
英文摘要A tau lepton can be produced in a charged current interaction by a cosmic ray tau neutrino with material inside a mountain. If it escapes from the mountain, it will decay and initiate a shower in the air, which can be detected by an air shower fluorescence/Cherenkov light detector. Designed according to such a principle, the cosmic ray tau neutrino telescope (CRTNT) experiment, located at the foothill of Mt Balikun in Xinjiang, China, will search for very high-energy cosmic tau neutrinos from energetic astrophysical sources by detecting those showers. This paper describes a Monte Carlo simulation for a detection of t events by the CRTNT experiment. Ultra-high-energy cosmic ray events are also simulated to estimate the potential contamination. With the CRTNT experiment composed of four detector stations, each covering 64 degrees x 14 degrees field of view, the expected event rates are 28.6, 21.9 and 4.7 per year assuming an AGN neutrino flux according to Semikoz and Sigl (2004 J. Cosmol. Astropart. Phys. JCAP 04(2004)003), Mannheim-Protheroe-Rachen (MPR) active galactic nucleus (AGN) jet model and Stecker-Done-Salamon-Sommers (SDSS) AGN core model, respectively. Null detection of such a tau event by the CRTNT experiment in 1 year could set a 90% C. L. upper limit on 19.9 (eV cm(-2) s(-1) sr(-1)) for an E(-2) neutrino spectrum.
类目[WOS]Physics, Nuclear ; Physics, Particles & Fields
研究领域[WOS]Physics
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语种英语
WOS记录号WOS:000266577700016
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文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/240796
专题中国科学院高能物理研究所_粒子天体物理中心_期刊论文
中国科学院高能物理研究所_粒子天体物理中心
中国科学院高能物理研究所_理论物理室
中国科学院高能物理研究所_大装置管理中心
作者单位中国科学院高能物理研究所
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Liu JL,Zhang SS,Cao Z,et al. Simulation of the cosmic ray tau neutrino telescope (CRTNT) experiment[J]. JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS,2009,36(7):75201.
APA 刘加丽.,张寿山.,曹臻.,何会海.,肖刚.,...&Zhang, Y.(2009).Simulation of the cosmic ray tau neutrino telescope (CRTNT) experiment.JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS,36(7),75201.
MLA 刘加丽,et al."Simulation of the cosmic ray tau neutrino telescope (CRTNT) experiment".JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS 36.7(2009):75201.
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