Reexamination of cosmic-ray composition around 10(18) eV from Fly's Eye data
文献类型:期刊论文
作者 | Ding LK(丁林恺); Jing CL(经才骝); Jing GR(荆贵茹); Ren JL(任江龙); Zhu QQ(朱清棋); Ding, LK; Jing, CL; Jing, GR; Ren, JL; Zhu, QQ |
刊名 | ASTROPHYSICAL JOURNAL
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出版日期 | 1997 |
卷号 | 474期号:1页码:490-495 |
关键词 | cosmic rays instrumentation, detectors |
通讯作者 | UNIV UTAH,INST HIGH ENERGY ASTROPHYS,SALT LAKE CITY,UT 84112 |
英文摘要 | The cosmic-ray composition around 10(18) eV is reexamined using the Chou-Yang model for the simulation of air showers and comparing with Fly's Eye data. This model is quite different from models previously used. Using this model leads to the same conclusion that the primary cosmic-ray composition gets lighter in the region from 3 x 10(17) eV to 10(19) eV. This conclusion of a changing composition is not sensitive to the choice of model because it results from the measured elongation rate being greater than that predicted for a constant composition by any reasonable model that can account for the measured depths of shower maxima at the Fly's Eye threshold energy. That constraint on elongation rate for a constant composition also implies that the increased rate of energy dissipation that appears in hadron-nucleus interactions near 10(14) eV may continue up to the region of 10(19) eV. |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
原文出处 | SCI |
语种 | 英语 |
WOS记录号 | WOS:A1997WA68200039 |
源URL | [http://ir.ihep.ac.cn/handle/311005/237698] ![]() |
专题 | 高能物理研究所_粒子天体物理中心 |
作者单位 | 中国科学院高能物理研究所 |
推荐引用方式 GB/T 7714 | Ding LK,Jing CL,Jing GR,et al. Reexamination of cosmic-ray composition around 10(18) eV from Fly's Eye data[J]. ASTROPHYSICAL JOURNAL,1997,474(1):490-495. |
APA | 丁林恺.,经才骝.,荆贵茹.,任江龙.,朱清棋.,...&Tang, JKK.(1997).Reexamination of cosmic-ray composition around 10(18) eV from Fly's Eye data.ASTROPHYSICAL JOURNAL,474(1),490-495. |
MLA | 丁林恺,et al."Reexamination of cosmic-ray composition around 10(18) eV from Fly's Eye data".ASTROPHYSICAL JOURNAL 474.1(1997):490-495. |
入库方式: OAI收割
来源:高能物理研究所
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