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100 TeV diffuse γ-rays observation by YangBaJing Hybrid Array

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摘要 Purpose Cosmic rays up to PeV energy are believed to be generated in our galaxy.γ-rays at 100TeV energies are important probe to identify PeVtrons.Besides,γ-rays contain additional information on the propagation of the galactic cosmic rays.Methods Diffuseγ-rays originating from the Galactic plane from 20 to 200 TeV region are studied with early 160-day data collected by YangBaJing Hybrid Array(YBJ-HA),which is a hybrid array and consists of scintillation detectors and underground muon detectors.All-distance equi-zenith angle and time-swapping methods are used to analyze the number ofγ-rays excess.Result and conclusion Because of no significant observation onγ-ray emission,Helene's method is adopted to derive the 90%confidence level upper limits on the flux of diffuse galacticγ-rays.And the limit to the ratio of the flux ofγ-rays to CRs is obtained at the order of 10^(-4),which is the current best result at these energies.
作者 Jian-Cheng He Yu-Hua Yao Zhen Wang Tian-Lu Chen Dan-Zeng-Luo-Bu Cun-Feng Feng Youliang Feng Qi Gao Yi-Qin Guo Ying-Ying Guo Hong-Bo Hu Xing-Tao Huang Cheng Liu Mao-Yuan Liu Yi-Bin Pan Bing-Qiang Qiao Guang-Guang Xin Xue-Yao Zhang Yi Zhang Shi-Ping Zhao
机构地区 Key Laboratory of Particle Astrophysics University of Chinese Academy of Sciences(UCAS) College of Physics Tsung-Dao Lee Institute Physics Department of Science School Institute of Frontier and Interdisciplinary Science Key Laboratory of Dark Matter and Space Astronomy Department of Physics School of Physics and Technology
出处 《Radiation Detection Technology and Methods》 CSCD 2020年第3期392-398,共7页 辐射探测技术与方法（英文）
基金 supported by National Natural Science Foundation of China under grant:11635011,11761141001,11873005,11765019,11963004
关键词 Cosmic rays Diffuse y-rays YBJ-HA EAS
分类号 O57 [理学—粒子物理与原子核物理]
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  • 1J. A. Simpson and M. Garcia-Mufioz, Space Sci. Rev., 1988, 46(3-4): 205. 被引量：1
  • 2M. A. Malkov and L. O. C. Drury, Rep. Prog. Phys., 2001, 64(4): 421. 被引量：1
  • 3A. Obermeier, P. Boyle, J. HSrandel, and D. Miiller, Astro- phys. J., 2012, 752(1): 69. 被引量：1
  • 4M. Ackermann, et al. [Fermi Collaboration], Astrophys. J., 2012, 750:3. 被引量：1
  • 5J. Holder, Astropart. Phys., 2012, 39-40:61. 被引量：1
  • 6E. S. Seo, Astropart. Phys., 2012, 39 40:76. 被引量：1
  • 7H. S. Ahn, et al. [CREAM Collaboration], Astrophys. J., 2009, 707:593. 被引量：1
  • 8H. S. Ahn, et al. [CREAM Collaboration], Astrophys. J., 2010, 714:L89. 被引量：1
  • 9O. Adriani, et al. [Pamela Collaboration], Science, 2011, 332: 69. 被引量：1
  • 10K. Asakimori, T. H. Burnett~ M. L. Cherry, K. Chevli, et al., Astrophys. J., 1998, 502(1): 278. 被引量：1

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  • 2Cliuan Yue,Peng-Xiong Ma,Qiang Yuan,Yi-Zhong Fan,Zhan-Fang Chen,Ming-Yang Cui,Hao-Ting Dai,Tie-Kuang Dong,Xiaoyuan Huang,Wei Jiang,Shi-Jun Lei,Xiang Li,Cheng-Ming Liu,Hao Liu,Yang Liu,Chuan-Ning Luo,Xu Pan,Wen-Xi Peng,Rui Qiao,Yi-Feng Wei,Li-Bo Wu,Zhi-Hui Xu,Zun-Lei Xu,Guan-Wen Yuan,Jing-Jing Zang,Ya-Peng Zhang,Yong-Jie Zhang,Yun-Long Zhang.Implications on the origin of cosmic rays in light of 10 TV spectral softenings[J].Frontiers of physics,2020,15(2):101-109. 被引量：2
  • 3F.Aharonian,V.Alekseenko,Q.An,Axikegu,L.X.Bai,Y.W.Bao,D.Bastieri9,X.J.Bi,H.Cai,Zhe Cao,Zhen Cao,J.Chang,J.F.Chang,X.C.Chang,S.P.Chao,B.M.Chen,J.Chen,L.Chen,L.Chen,M.L.Chen,M.J.Chen,Q.H.Chen,S.H.Chen,S.Z.Chen,T.L.Chen,X.L.Chen,Y.Chen,N.Cheng,Y.D.Cheng,S.W.Cui,X.H.Cui,Y.D.Cui,B.Z.Dai,H.L.Dai,Z.G.Dai,Danzengluobu,B.D'Ettorre Piazzoli,J.Fang,J.H.Fan,Y.Z.Fan,C.F Feng,L.Feng,S.H.Feng,Y.L.Feng,B.Gao,Q.Gao,W.Gao,M.M.Ge,L.S.Geng,G.H.Gong,Q.B.Gou,M.H.Gu,Y.Q.Guo,Y.Y.Guo,Y.A.Han,H.H.He,J.C.He,M.Heller,S.L.He,Y.He,C.Hou,D.H.Huang,Q.L.Huang,W.H.Huang,X.T.Huang,H.B.Hu,S.Hu,H.Y.Jia,K.Jiang,F.Ji,C.Jin,X.L.Ji,K.Levochkin,E.W.Liang,Y.F Liang,Cheng Li,Cong Li,F.Li,H.Li,H.B.Li,H.C.Li,H.M.Li,J.Li,K.Li,W.L.Li,X.Li,X.R.Li,Y.Li,Z.Li,Z.Li,B.Liu,C.Liu,D.Liu,H.D.Liu,H.Liu,J.Liu,J.Y.Liu,M.Y.Liu,R.Y.Liu,S.M.Liu,W.Liu,Y.N.Liu,Z.X.Liu,W.J.Long,R.Lu,H.K.Lv,B.Q.Ma,L.L.Ma,J.R.Mao,A.Masood,X.H.Ma,W.Mitthumsiri,T.Montaruli,Y.C.Nan,P.Pattarakijwanich,Z.Y.Pei,B.Q.Qiao,M.Y.Qi,D.Ruffolo,V.Rulev,A.Sáiz,L.Shao,O.Shchegolev,X.D.Sheng,J.R.Shi,Y.Stenkin,V.Stepanov,Z.B.Sun,P.H.T.Tam,Z.B.Tang,W.W.Tian,D.D.Volpe,C.Wang,H.Wang,H.G.Wang,J.C.Wang,L.Y.Wang,W.Wang,W.Wang,X.G.Wang,X.Y.Wang,X.J.Wang,Y.D.Wang,Y.J.Wang,Y.N.Wang,Y.P.Wang,Z.Wang,Z.H.Wang,Z.X.Wang,D.M.Wei,J.J.Wei,T.Wen,C.Y.Wu,H.R.Wu,S.Wu,W.X.Wu,X.F.Wu,G.M.Xiang,G.Xiao,G.G.Xin,Y.Xing,R.X.Xu,L.Xue,D.H.Ya.Prospects for a multi-TeV gamma-ray sky survey with the LHAASO water Cherenkov detector array[J].Chinese Physics C,2020,44(6):123-132.
  • 4郑应,何钰,祝凤荣,张丰.基于地面粒子探测器阵列的一种新芯位重建方法[J].天文研究与技术,2023,20(5):478-486.
  • 5Bing-Bing Li,Xin-Hua Ma,Shu-Wang Cui,Hao-Kun Chen,Tian-Lu Chen,Danzengluobu,Wei Gao,Hai-Bing Hu,Denis Kuleshov,Kirill Kurinov,Hu Liu,Mao-Yuan Liu,Ye Liu,Da-Yu Peng,Yao-Hui Qi,Oleg Shchegolev,Yuri Stenkin,Li-Qiao Yin,Heng-Yu Zhang,Liang-Wei Zhang.Research on the knee region of cosmic ray by using a novel type of electron-neutron detector array[J].Frontiers of physics,2024,19(4):13-24.
Radiation Detection Technology and Methods
2020年 第3期

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