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已选条件: 数据来源: 维普 × 数据来源: WOS × 数据来源: CNKI × 数据来源: 万方 × 出版年: 2000 × 出版物中文: 高能物理与核物理 × 机构: 物理学院 ×
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gamma gamma V(rho, phi) have been studied. The eta(1430) resonance has been observed in these two channels respectively. Its mass,width and branching ratio are 1431 +/- 17MeV, 88 +/- 28MeV, and Br (J/psi-->gamma eta(1430)) Br(eta(1430)-->gamma rho) = (1.1 +/- 0.5 +/- 0.3) x 10(-4) from J/psi-->gamma gamma rho mode,1424 +/- 15MeV, 73 +/- 58MeV, and Br(J/psi-->gamma eta(1430)) Br(eta(1430)-->gamma phi) = (2.0 +/- 1.0 +/- 0.6) x 10(-4) from J/psi-->gamma gamma phi mode. [researcherID] => Hong, Tao/F-8166-2010 [orcID] => Hong, Tao/0000-0002-0161-8588 [article_dt] => Article [publication_type] => J [begin_page] => 892 [author_en] => Bai, JZ; Ban, Y; Bian, JG; Chen, AD; Chen, GP; Chen, HF; Chen, HS; Chen, JC; Chen, XD; Chen, YB; Chen, BS; Chu, YP; Cui, XZ; Ding, HL; Dai, YS; Dong, LY; Du, ZZ; Gao, CS; Gao, SQ; Gu, SD; Guo, YN; Guo, ZJ; Han, SW; Han, Y; He, JT; He, J; He, KL; He, M; He, X; Heng, YK; Hong, T; Hu, GY; Hu, HM; Hu, JL; Hu, QH; Hu, T; Huang, GS; Huang, XP; Huang, YZ; Jiang, CH; Jin, Y; Ju, X; Ke, ZJ; Lai, YF; Lang, PF; Li, CG; Li, D; Li, HB; Li, JC; Li, J; Li, PQ; Li, QJ; Li, RY; Li, W; Li, WG; Li, XN; Li, XH; Li, XQ; Li, ZC; Liu, B; Liu, F; Liu, HM; Liu, J; Liu, JP; Liu, RG; Liu, Y; Liu, ZX; Liu, F; Lu, GR; Lu, F; Lu, JG; Lu, ZJ; Luo, XL; Ma, EC; Ma, JM; Mao, HS; Mao, ZP; Meng, XC; Mo, XH; Nie, J; Nie, ZD; Qi, ND; Qi, XR; Qian, CD; Qiu, JF; Que, YK; Rong, G; Shao, YY; Shen, BW; Shen, DL; Shen, H; Shen, XY; Shen, HY; Shi, F; Shi, HZ; Song, XF; Sun, HS; Sun, LF; Sun, YZ; Tang, SQ; Tong, GL; Wang, JZ; Wang, J; Wang, L; Wang, LZ; Wang, LS; Wang, PL; Wang, P; Wang, SM; Wang, YY; Wang, ZY; Wei, CL; Wu, N; Wu, YG; Xi, DM; Xia, XM; Xie, XX; Xie, YH; Xu, GF; Xue, ST; Yan, WG; Yang, CY; Yang, CM; Yang, GA; Yang, HX; Yang, XF; Ye, MH; Ye, SW; Ye, YX; Yu, CS; Yu, CX; Yu, GW; Yu, ZQ; Yuan, Y; Zhang, BY; Zhang, CC; Zhang, C; Zhang, DH; Zhang, HL; Zhang, J; Zhang, JW; Zhang, LS; Zhang, L; Zhang, L; Zhang, QJ; Zhang, SQ; Zhang, XY; Zhang, YY; Zhang, ZP; Zhang, HY; Zhang, P; Zhao, DX; Zhao, HW; Zhao, JW; Zhao, JW; Zhao, M; Zhao, PP; Zhao, WR; Zhao, YB; Zhao, ZG; Zheng, JP; Zheng, LS; Zheng, ZP; Zhou, BQ; Zhou, GM; Zhou, L; Zhu, KJ; Zhu, QM; Zhu, YS; Zhu, ZA; Zhu, YC; Zhuang, BA; Zou, BS [volume] => 24 [publisher] => SCIENCE PRESS [get_data] => 2018-08-29 [keyword_en] => J/Psi; resonance; meson; glueball [page] => 892-900 [keyword_plu] => GEV/C [format_publication_cn] => 1e4ba0a3cae0934c4c5e0c2149a71c3c35052158 [publication_iso] => High Energy Phys. Nucl. Phys.-Chin. Ed. [format_title_en_publication_en_pub_year] => 3dc391d3bce67c56c80524a950eb8fb1-529682636 [format_title_en] => a02c2785567f79579c927e429523f89c1655850816 [publisher_city] => BEIJING [pub_date] => OCT [cauthor_order] => 1 [hx_id] => 2371 [reference_No] => 11 [format_issn_issue_page_pub_year] => 731a5db879afa37f364950e9d37e17fb-1282318901 [cite_awos] => 0 [wos_No] => WOS:000089929500002 [format_wos_No] => b9d29e7ed057720608a5fafb249dfeae809277798 [wos_sub] => Physics, Nuclear; Physics, Particles & Fields [research_area] => Physics [cauthor_back] => Bai, JZ [check_180] => 0 [publisher_ad] => 16 DONGHUANGCHENGGEN NORTH ST, BEIJING 100717, PEOPLES R CHINA [title_en] => Study of decay J/Psi ->gamma gamma V(rho,phi) [format_publication_en] => 447a5ff97055faf0b52669582cc267d5690401559 [jl_article_dt] => 期刊论文 [id] => _QkwvmUBFjIhTVEb6M9i [tags] => 0 ) [4] => Array ( [batch2] => 2 [uri] => http://kns.cnki.net/kns/detail/detail.aspx?FileName=KNWL200011000&DbName=CJFQ2000 [tag] => 0 [abstract_cn] => 通过对甘巴拉山K0—K7乳胶室所观测到的部分族事例与运用COSMOS, CORSIKA程序产生的模拟族事例进行了可分辨能量中心(EDC)的共线性的分 析,结果表明:在实验族事例中,共线事例产生的份额随族的总观测能的增高而上 升;而传统的模拟计算不能解释共线现象这一特征.文中还对族事例中γ线与强 子的判别标准进行了讨论. [keyword_cn] => 乳胶室;;γ-强子族;;Monte Carlo模拟;;共线性 [fund_No] => 国家自然科学基金!(19875031);;高等学校博士学科点专项科研基金 [article_id] => 28195,595376 [clc] => O571 [author_jg] => [薛良]山东大学物理系!济南250100@@@[戴志强]山东大学物理系!济南250100@@@[李金玉]山东大学物理系!济南250100@@@[张学尧]山东大学物理系!济南250100@@@[冯存峰]山东大学物理系!济南250100@@@[傅宇]山东大学物理系!济南250100@@@[张乃健]山东大学物理系!济南250100@@@[任敬儒]中国科学院高能物理研究所!北京100039@@@[陆穗苓]中国科学院高能物理研究所!北京100039 [format_title_cn_publication_cn_pub_year] => db0e22ef3c6d8f2bcd241d608d2cdb85-210992647 [hints] => 9 [issue] => 11 [author_first] => 薛良 [sys_level_num] => 2_3 [sys_jg_type] => 0 [format_issn_issue_page_pub_year] => f6f45d7f3ecee7fd055a4e33b370b68e1137398101 [source_type] => 351 [pub_year] => 2000 [pub_date] => 2000-11-15 [pages] => 979-984 [from_id] => 85,78 [author_cn] => 薛良;戴志强;李金玉;张学尧;冯存峰;傅宇;张乃健;任敬儒;陆穗苓 [issn] => 1674-1137 [batch] => 3250,3254 [publication_cn] => 高能物理与核物理 [title_cn] => 宇宙线高能族事例中的共线现象 [CSSN] => 11-5641/O4 [SYS_TAG] => 3 [format_title_cn_issn_pub_year] => 77c65681a3c9f8433965a9f8805f4aa9-273202710 [page] => 979-984 [hb_type] => 2 [article_dt] => 期刊论文 [hb_batch] => title_cn_publication_cn_pub_year_2_3 [format_title_en] => [format_title] => 1ecf4601c7358d815f438ead37ffa754-1644100175 [hx_id] => [format_publication_cn] => 1e4ba0a3cae0934c4c5e0c2149a71c3c35052158 [format_publication_en] => [jl_publication_cn] => 高能物理与核物理 [jl_article_dt] => 期刊论文 [jl_country] => 中国 [jl_keyword_cn] => ,montecarlo模拟,乳胶室,γ强子族,共线性 [jl_clc] => o571 [author_in] => [author_id] => 20699,24876,25735 [author_test] => Array ( [0] => Array ( [sure] => 1 [irmagnum] => 0 [u_index] => 5 [name] => 冯存峰 [irtag] => 0 [t_index] => 0 [person_id] => 20699 ) [1] => Array ( [sure] => 1 [irmagnum] => 0 [u_index] => 1 [name] => 薛良 [irtag] => 0 [t_index] => 0 [person_id] => 24876 ) [2] => Array ( [sure] => 1 [irmagnum] => 0 [u_index] => 4 [name] => 张学尧 [sys_author_id] => Array ( [0] => 20699 [1] => 24876 [2] => 25735 ) [irtag] => 0 [t_index] => 0 [person_id] => 25735 ) ) [company_id] => 133,5 [sys_subject_sort] => 0,0 [college_parent_id] => 133,5 [company_test] => Array,Array [sys_author_id_arr] => 20699冯存峰,24876薛良,25735张学尧 [jl_publication_cn_publication_en] => 高能物理与核物理 [jl_keyword_cn_keyword_en] => γ强子族,montecarlo模拟,乳胶室,共线性 [sys_author_id] => 20699,24876,25735 [id] => _w5HvmUBFjIhTVEbgCnH [tags] => 0 ) [5] => Array ( [issn] => 0254-3052 [delivery_No] => 333TF [batch2] => 1,2,6 [hb_batch] => 3241 [tag] => 0 [author_en] => Xu, XW; Ding, LK; Cao, PY; Dai, BZ; Feng, ZY; Fu, Y; Guo, HW; He, M; Huang, Q; Huo, AX; Jia, HY; Li, JY; Liu, SM; Lu, H; Lu, SL; Luo, GX; Mei, DM; Meng, XR; Mu, J; Peng, ZR; Ren, JR; Shi, C; Shi, ZZ; Tan, YH; Wang, CR; Wang, H; Yu, GC; Yuan, AF; Zhang, CS; Zhang, HM; Zhang, JL; Zhang, NJ; Zhang, XY; Zhaxisangzhu; Zhaxiciren; Zhou, WD [abstract_en] => A lot of data has been accumulated with Tibet II and HD AS array operated successfully since October of 1995 and 1996, respectivley. The preliminary results of searching for steady TeV gamma ray emissions from Crab Nebula with these data were presented in this paper. Analysis shows that the accumulative excess events of steady 3TeV gamma ray emissions from Crab Nebula was increasing stably and the statistical significance reached 3.2 sigma, whereas no statistical significant evidence of steady 10TeV and 30TeV gamma ray emissions was found. [publication_type] => J [keyword_plu] => CERENKOV IMAGING TECHNIQUE; SPECTRUM [author_in] => [Xu, X.W] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Ding, L.K] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Cao, P.Y] Department of Physics, Shangdong University, Ji\' nan 250100, China@@@[ Dai, B.Z] Department of Physics, Yunnan University, Kunming 650091, China@@@[ Feng, Z.Y] Department of Physics, South West Jiaotong University, Chengdu 610031, China@@@[ Fu, Y] Department of Physics, Shangdong University, Ji\' nan 250100, China@@@[ Guo, H.W] Dept. of Mathematics and Physics, Tibet University, Lhasa 850000, China@@@[ He, M] Department of Physics, Shangdong University, Ji\' nan 250100, China@@@[ Huang, Q] Department of Physics, South West Jiaotong University, Chengdu 610031, China@@@[ Huo, A.X] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Jia, H.Y] Department of Physics, South West Jiaotong University, Chengdu 610031, China@@@[ Li, J.Y] Department of Physics, Shangdong University, Ji\' nan 250100, China@@@[ Liu, S.M] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Lu, H] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Lu, S.L] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Luo, G.X] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Mei, D.M] Dept. of Mathematics and Physics, Tibet University, Lhasa 850000, China@@@[ Meng, X.R] Dept. of Mathematics and Physics, Tibet University, Lhasa 850000, China@@@[ Mu, J] Department of Physics, Yunnan University, Kunming 650091, China@@@[ Peng, Z.R] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Ren, J.R] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Shi, C] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Shi, Z.Z] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Tan, Y.H] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Wang, C.R] Department of Physics, Shangdong University, Ji\' nan 250100, China@@@[ Wang, H] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Yu, G.C] Department of Physics, South West Jiaotong University, Chengdu 610031, China@@@[ Yuan, A.F] Dept. of Mathematics and Physics, Tibet University, Lhasa 850000, China@@@[ Zhang, C.S] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Zhang, H.M] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Zhang, J.L] Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China@@@[ Zhang, N.J] Department of Physics, Shangdong University, Ji\' nan 250100, China@@@[ Zhang, X.Y] Department of Physics, Shangdong University, Ji\' nan 250100, China@@@[ Zhaxisangzhu Dept. of Mathematics and Physics] Tibet University, Lhasa 850000, China@@@[ Zhaxiciren Dept. of Mathematics and Physics] Tibet University, Lhasa 850000, China@@@[ Zhou, W.D] Department of Physics, Yunnan University, Kunming 650091, China [publisher_city] => BEIJING [cauthor_back] => Xu, XW [get_data] => 2018-08-29 [format_title_en_publication_en_pub_year] => 5b1c1410df7188f2ae1f67c58722a19b334907217 [begin_page] => 473 [cite_wos] => 1 [check_3Y] => 1 [cite_awos] => 1 [from_id] => 76,80,78,73,85 [cauthor_ad] => [Xu, XW]Chinese Acad Sci, Inst High Energy Phys, Key Lab Cosm Ray & High Energy Astrophys, Beijing 100039, Peoples R China. [school_id] => 117 [cauthor_order] => 1 [research_area] => Physics [sys_level_num] => 1_7 [publisher] => SCIENCE PRESS [sys_jg_type] => 10,3,5 [format_issn_issue_page_pub_year] => 938358ac25754cfcbba64e3579b46797-728537167 [title_en] => Search for TeV gamma rays from the Crab Nebula with Tibet II HD AS array [publication_29] => HIGH ENERG PHYS NUC [author_fn] => Xu, XW; Ding, LK; Cao, PY; Dai, BZ; Feng, ZY; Fu, Y; Guo, HW; He, M; Huang, Q; Huo, AX; Jia, HY; Li, JY; Liu, SM; Lu, H; Lu, SL; Luo, GX; Mei, DM; Meng, XR; Mu, J; Peng, ZR; Ren, JR; Shi, C; Shi, ZZ; Tan, YH; Wang, CR; Wang, H; Yu, GC; Yuan, AF; Zhang, CS; Zhang, HM; Zhang, JL; Zhang, NJ; Zhang, XY; Zhaxisangzhu; Zhaxiciren; Zhou, WD [pub_year] => 2000 [publisher_ad] => 16 DONGHUANGCHENGGEN NORTH ST, BEIJING 100717, PEOPLES R CHINA [check_180] => 0 [keyword_en] => cosmic ray; air shower; gamma ray astronomy; gamma ray source [end_page] => 477 [pub_date] => JUN [pages] => 5 [format_wos_No] => 7ece2dbff2fbbc64f001a6baef800cc3-2108110285 [hints] => 14 [volume] => 24 [language] => Chinese [source_type] => 351 [issue] => 6 [reference_No] => 10 [batch] => 3243,3250,3241,3254,3252 [publication_en] => HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION [hx_id] => 2378,2371 [sys_update_time] => 2018-09-05 15:29:30 [format_title_en_issn_pub_year] => 237c310a102b63347698e683d0a9c99d-1842150049 [publication_iso] => High Energy Phys. Nucl. Phys.-Chin. Ed. [article_id] => 333593,167559,595379,497115,65892 [wos_sub] => Physics, Nuclear; Physics, Particles & Fields [SYS_TAG] => 3 [wos_No] => WOS:000088146300002 [page] => 473-477 [hb_type] => 2 [article_dt] => Article [jl_language] => chinese [jl_article_dt] => 期刊论文 [jl_publication_en] => highenergyphysicsandnuclearphysicschineseedition [jl_country] => 中国 [jl_keyword_en] => gammaraysource,airshower,gammarayastronomy,cosmicray [jl_publisher] => sciencepress [author_jg] => [许贤武,丁林恺,曹培园,戴本忠,冯振勇,傅宇,郭宏伟,何瑁,黄庆,霍安祥,贾焕玉,李金玉,刘绍敏,卢红,陆穗玲,罗光宣,梅东明,孟宪茹,木钧,彭朝然,任敬儒,史策,施志政,谭有恒,王承瑞,王辉,余光策,袁爱芳,张春生,张慧敏,张吉龙,张乃健,张学尧,扎西桑珠,扎西次仁,周文德]中国科学院高能物理研究所宇宙线和高能天体物理开放实验室!北京100039,中国科学院高能物理研究所宇宙线和高能天体物理开放实验室!北京100039,山东大学物理系!济南250100,云南大学物理系!昆明650091,西南交通大学物理系!成都610031,山东大学物理系!济南250100,西藏大学数理系! [keyword_cn] => 宇宙射线;大气簇射;γ射线天文学;γ射线源 [format_title] => 972dde151c106d932400f775e6f23dcc-446252045 [cite_wanfang] => 4 [clc] => O572.12 [title_cn] => TibetⅡ/HD阵列寻找来自蟹状星云的TeVγ射线 [format_publication_cn] => 1e4ba0a3cae0934c4c5e0c2149a71c3c35052158 [publication_cn] => 高能物理与核物理 [format_title_en] => ce9ddd3e5c3899b9d580f49001416897767000847 [CSSN] => 11-5641/O4 [abstract_cn] => 羊八井二期阵列 (TibetⅡ )和加密阵列HD(HighDensity)分别从 1 995年和 1 996年成功地运行以来 ,已经积累了大量的数据 .报道了利用TibetⅡ在1 995年 1 0月至 1 997年 9月、HD阵列在 1 997年 2月至 8月收集的数据寻找来自蟹状星云 (CrabNebula)方向的 1 0TeV和 3TeVγ射线稳定发射的初步结果 .分析表明 ,来自CrabNebula的 3TeVγ射线的累积信号事例数显示了稳定增长的趋势 ,显著性达到了 3.2σ,但没有发现 1 0TeV和 30TeVγ射线稳定发射的迹象 [sys_priority_field] => 76 [author_cn] => 许贤武,丁林恺,曹培园,戴本忠,冯振勇,傅宇,郭宏伟,何瑁,黄庆,霍安祥,贾焕玉,李金玉,刘绍敏,卢红,陆穗玲,罗光宣,梅东明,孟宪茹,木钧,彭朝然,任敬儒,史策,施志政,谭有恒,王承瑞,王辉,余光策,袁爱芳,张春生,张慧敏,张吉龙,张乃健,张学尧,扎西桑珠,扎西次仁,周文德 [format_publication_en] => 447a5ff97055faf0b52669582cc267d5690401559 [jl_publication_cn] => 高能物理与核物理 [jl_keyword_cn] => γ射线天文学,宇宙射线,大气簇射,γ射线源 [jl_clc] => o57 [company_id] => 133,0,5 [author_id] => 25353,25408,25720,25428,25689,25444,22406,23932,23933,24792,23910,23911,25719,25414,25735,22416,22414,25692,23919,23921,23920,23922,26122 [author_test] => Array ( [0] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 31 [name] => 张家良 [irtag] => 7 [t_index] => 0 [person_id] => 25444 ) [1] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 26 [name] => 王辉 [irtag] => 7 [t_index] => 0 [person_id] => 23933 ) [2] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 26 [name] => 王灏 [irtag] => 7 [t_index] => 0 [person_id] => 23910 ) [3] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 26 [name] => 王红 [irtag] => 7 [t_index] => 0 [person_id] => 23911 ) [4] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 1 [name] => 徐晓文 [irtag] => 7 [t_index] => 1 [person_id] => 24792 ) [5] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 33 [name] => 张熙颖 [irtag] => 7 [t_index] => 0 [person_id] => 25692 ) [6] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 26 [name] => 王辉 [irtag] => 7 [t_index] => 0 [person_id] => 23932 ) [7] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 30 [name] => 张红梅 [irtag] => 7 [t_index] => 0 [person_id] => 25414 ) [8] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 13 [name] => 刘尚明 [irtag] => 7 [t_index] => 0 [person_id] => 22406 ) [9] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 26 [name] => 王华 [irtag] => 7 [t_index] => 0 [person_id] => 23921 ) [10] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 13 [name] => 刘守民 [irtag] => 7 [t_index] => 0 [person_id] => 22416 ) [11] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 26 [name] => 王华 [irtag] => 7 [t_index] => 0 [person_id] => 23922 ) [12] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 26 [name] => 王华 [irtag] => 7 [t_index] => 0 [person_id] => 23919 ) [13] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 13 [name] => 刘世明 [irtag] => 7 [t_index] => 0 [person_id] => 22414 ) [14] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 29 [name] => 张存生 [irtag] => 7 [t_index] => 0 [person_id] => 25353 ) [15] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 33 [name] => 张晓阳 [irtag] => 7 [t_index] => 0 [person_id] => 25720 ) [16] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 33 [name] => 张行愚 [irtag] => 7 [t_index] => 0 [person_id] => 25408 ) [17] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 36 [name] => 周卫东 [irtag] => 7 [t_index] => 0 [person_id] => 26122 ) [18] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 33 [name] => 张晓燕 [irtag] => 7 [t_index] => 0 [person_id] => 25719 ) [19] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 30 [name] => 张华梅 [irtag] => 7 [t_index] => 0 [person_id] => 25428 ) [20] => Array ( [sure] => 1 [irmagnum] => 0 [u_index] => 33 [name] => 张学尧 [irtag] => 0 [t_index] => 0 [person_id] => 25735 ) [21] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 26 [name] => 王华 [irtag] => 7 [t_index] => 0 [person_id] => 23920 ) [22] => Array ( [sure] => 0 [irmagnum] => 0 [u_index] => 33 [name] => 张锡宇 [sys_author_id] => Array ( [0] => 25735 ) [irtag] => 7 [t_index] => 0 [person_id] => 25689 ) ) [sys_author_id_arr] => 25735张学尧 [jl_publication_cn_publication_en] => highenergyphysicsandnuclearphysicschineseedition,高能物理与核物理 [jl_keyword_cn_keyword_en] => airshower,gammarayastronomy,gammaraysource,大气簇射,cosmicray,宇宙射线,γ射线天文学,γ射线源 [datebase] => Scopus [format_scopus_No] => be7cf4f413059515d37116b4741e9aa51943047208 [classification_pub] => KNWLD [uri] => http://kns.cnki.net/kns/detail/detail.aspx?FileName=KNWL200006001&DbName=CJFQ2000 [standard_in] => Key Lab. Cosmic Ray High Ener. A., Institute of High Energy Physics, CAS, Beijing 100039, China; Department of Physics, Shangdong University, Ji\' nan 250100, China; Department of Physics, Yunnan University, Kunming 650091, China; Department of Physics, South West Jiaotong University, Chengdu 610031, China; Dept. of Mathematics and Physics, Tibet University, Lhasa 850000, China [scopus_No] => 2-s2.0-20244378649 [format_title_cn_publication_cn_pub_year] => cb202d69901d03aa892c25134ef3f0a11177968961 [format_title_cn_issn_pub_year] => f85a7818d9a2270c5a92160c85d759d4-1430392715 [jl_author_test] => upersonid23911,usureu0,unameuu738bu8f89,unameuu738bu534e,unameuu5218u5b88u6c11,unameuu738bu7ea2,upersonid23921,unameuu5f20u9521u5b87,unameuu5218u5c1au660e,uirauthortype0,uirauthortype3,upersonid23932,upersonid23933,upersonid22406,upersonid23919,unameuu5218u4e16u660e,upersonid26122,uirtstag0,upersonid25353,unameuu5f20u6653u71d5,upersonid25414,unameuu5f20u5b66u5c27,upersonid25719,uuindex13,unameuu5f20u7199u9896,uuindex33,uuindex30,upersonid25735,uuindex36,unameuu5468u536bu4e1c,unameuu5f20u5b58u751f,uuindex1,unameuu5f20u7ea2u6885,unameuu5f20u884cu611a,utindex0,uirtag7,uirinspecttag0,utindex1,upersonid24792,uirtag0,upersonid22416,upersonid23920,upersonid22414,upersonid23922,unameuu738bu704f,unameuu5f20u534eu6885,uirtypical1,uuindex31,upersonid25408,unameuu5f20u5bb6u826f,unameuu5f90u6653u6587,unameuu5f20u6653u9633,upersonid25689,uuindex29,upersonid25692,upersonid23910,upersonid25428,upersonid25444,upersonid25720,uuindex26 [sys_author_jg_last_arr] => 850000 [sys_author_in_last_arr] => china [sys_author_id] => 25735 [sys_subject_sort] => 0,0 [college_parent_id] => 133,5 [company_test] => Array,Array [id] => KAifvWUBFjIhTVEbTN9t [tags] => 0 ) ) 1-->
1. p—N(A)Drell—Yan过程K因子的非常数性和核环境影响 SCIE

作者:刘春秀[1];彭宏安[2];等

作者机构:[刘春秀]山东大学物理系,济南250100,中国.;[彭宏安]河北师范大学物理系,河北050016,中国

来源:高能物理与核物理,HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2000,Vol.24,Issue.2,131-139

WOS被引数:5

资源类型:期刊论文

WOS:000085719800007

2. 超高能γ-强子族的能量集中现象

作者:戴志强,薛良,李金玉,张学尧,冯存峰,傅宇,李婕,曹培园,张乃健,何瑁,王承瑞,任敬儒,陆穗苓

作者机构:[戴志强,薛良,李金玉,张学尧,冯存峰,傅宇,李婕,曹培园,张乃健,何瑁,王承瑞,任敬儒,陆穗苓]山东大学电子工程系!济南250100,山东大学物理系!济南250100,山东大学物理系!济南250100,山东大学物理系!济南250100,山东大学物理系!济南250100,山东大学物理系!济南250100,山东大学物理系!济南250100,山东大学物理系!济南250100,山东大学物理系!济南250100,山东大学物理系!济

来源:高能物理与核物理,2000,Issue.10,885-891

资源类型:期刊论文

3. 10TeVγ射线的星系际红外背景光子吸收现象的研究 SCIE

作者:许贤武,丁林恺,曹培圆,戴本忠,冯振勇,傅宇,郭宏伟,何瑁,黄庆,霍安祥,贾焕玉,李金玉,刘绍敏,卢红,陆穗苓,罗光宣,梅东明,孟宪茹,木钧,彭朝然,任敬儒,史策,施志政,谭有恒,王承瑞,王辉,余光策,袁爱芳,张春生,张慧敏,张吉龙,张乃健,张学尧,扎西桑珠,扎西次仁,周文德

作者机构:[许贤武,丁林恺,曹培圆,戴本忠,冯振勇,傅宇,郭宏伟,何瑁,黄庆,霍安祥,贾焕玉,李金玉,刘绍敏,卢红,陆穗苓,罗光宣,梅东明,孟宪茹,木钧,彭朝然,任敬儒,史策,施志政,谭有恒,王承瑞,王辉,余光策,袁爱芳,张春生,张慧敏,张吉龙,张乃健,张学尧,扎西桑珠,扎西次仁,周文德]中国科学院高能物理研究所宇宙线和高能天体物理开放实验室!北京100039,中国科学院高能物理研究所宇宙线和高能天体物理开放实验室!北京100039,山东大学物理系!济南250100,云南大学物理系!昆明650091,西南交通大学物理系!成都610031,西藏大学数理系!拉萨850000,西藏大学数理系!

来源:高能物理与核物理,HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2000,Vol.24,Issue.8,697-701

资源类型:期刊论文

WOS:000088798700001

4. J/Ψ→γγ(ρφ)衰变的实验研究 SCIE

作者:白景芝[1];何瑁[2];等

作者机构:[白景芝]中国科学院高能物理研究所,北京100039,中国.;[何瑁]山东大学物理系,济南250100,中国

来源:高能物理与核物理,HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2000,Vol.24,Issue.10,892-900

资源类型:期刊论文

WOS:000089929500002

5. 宇宙线高能族事例中的共线现象

作者:薛良;戴志强;李金玉;张学尧;冯存峰;傅宇;张乃健;任敬儒;陆穗苓

作者机构:[薛良]山东大学物理系!济南250100;[戴志强]山东大学物理系!济南250100;[李金玉]山东大学物理系!济南250100;[张学尧]山东大学物理系!济南250100;[冯存峰]山东大学物理系!济南250100;[傅宇]山东大学物理系!济南250100;[张乃健]山东大学物理系!济南250100;[任敬儒]中国科学院高能物理研究所!北京100039;[陆穗苓]中国科学院高能物理研究所!北京100039

来源:高能物理与核物理,2000,Issue.11,979-984

资源类型:期刊论文

6. TibetⅡ/HD阵列寻找来自蟹状星云的TeVγ射线 SCOPUS SCIE

作者:许贤武,丁林恺,曹培园,戴本忠,冯振勇,傅宇,郭宏伟,何瑁,黄庆,霍安祥,贾焕玉,李金玉,刘绍敏,卢红,陆穗玲,罗光宣,梅东明,孟宪茹,木钧,彭朝然,任敬儒,史策,施志政,谭有恒,王承瑞,王辉,余光策,袁爱芳,张春生,张慧敏,张吉龙,张乃健,张学尧,扎西桑珠,扎西次仁,周文德

作者机构:[许贤武,丁林恺,曹培园,戴本忠,冯振勇,傅宇,郭宏伟,何瑁,黄庆,霍安祥,贾焕玉,李金玉,刘绍敏,卢红,陆穗玲,罗光宣,梅东明,孟宪茹,木钧,彭朝然,任敬儒,史策,施志政,谭有恒,王承瑞,王辉,余光策,袁爱芳,张春生,张慧敏,张吉龙,张乃健,张学尧,扎西桑珠,扎西次仁,周文德]中国科学院高能物理研究所宇宙线和高能天体物理开放实验室!北京100039,中国科学院高能物理研究所宇宙线和高能天体物理开放实验室!北京100039,山东大学物理系!济南250100,云南大学物理系!昆明650091,西南交通大学物理系!成都610031,山东大学物理系!济南250100,西藏大学数理系!

来源:高能物理与核物理,HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2000,Vol.24,Issue.6,473-477

WOS被引数:1

资源类型:期刊论文

WOS:000088146300002

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