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Scattering Angle of Cosmic Ray Muons with Energy Loss Deep Underground
https://kindai.repo.nii.ac.jp/records/11179
https://kindai.repo.nii.ac.jp/records/11179e6649eca-fe52-477e-9360-8e97e71b3254
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
AN10074306-19900130-0081.pdf (596.8 kB)
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| Item type | ☆紀要論文 / Departmental Bulletin Paper(1) | |||||||||||||||||
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| 公開日 | 2015-03-10 | |||||||||||||||||
| タイトル | ||||||||||||||||||
| タイトル | Scattering Angle of Cosmic Ray Muons with Energy Loss Deep Underground | |||||||||||||||||
| 言語 | en | |||||||||||||||||
| 著者 |
Kitamura, Takashi
× Kitamura, Takashi
× Nakatsuka, Takao
× Kobayakawa, Keizo
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| 言語 | ||||||||||||||||||
| 言語 | eng | |||||||||||||||||
| キーワード | ||||||||||||||||||
| 主題 | Muon scatterings with energy loss and fluctuations, underground muons, SN1987A, high energy muons from Cygnus X-3 | |||||||||||||||||
| 資源タイプ | ||||||||||||||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||||||||||||||
| 資源タイプ | departmental bulletin paper | |||||||||||||||||
| 著者(英) | ||||||||||||||||||
| 言語 | en | |||||||||||||||||
| 値 | Kitamura, Takashi | |||||||||||||||||
| 著者(英) | ||||||||||||||||||
| 言語 | en | |||||||||||||||||
| 値 | Nakatsuka, Takao | |||||||||||||||||
| 著者(英) | ||||||||||||||||||
| 言語 | en | |||||||||||||||||
| 値 | Kobayakawa, Keizo | |||||||||||||||||
| 著者 所属 | ||||||||||||||||||
| 値 | Research Institute for Science and Technology, Kinki University | |||||||||||||||||
| 著者 所属 | ||||||||||||||||||
| 値 | Nagoya Women University | |||||||||||||||||
| 著者 所属 | ||||||||||||||||||
| 値 | Collage of Liberal Arts, Kobe University | |||||||||||||||||
| 著者所属(翻訳) | ||||||||||||||||||
| 値 | 近畿大学理工学総合研究所 | |||||||||||||||||
| 著者所属(翻訳) | ||||||||||||||||||
| 値 | 名古屋女子大学 | |||||||||||||||||
| 著者所属(翻訳) | ||||||||||||||||||
| 値 | 神戸大学 | |||||||||||||||||
| 版 | ||||||||||||||||||
| 出版タイプ | VoR | |||||||||||||||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||||||||||||||
| 出版者 名前 | ||||||||||||||||||
| 出版者 | 近畿大学理工学総合研究所 | |||||||||||||||||
| 書誌情報 |
理工学総合研究所研究報告 en : Annual reports by Research Institute for Science and Technology 巻 2, p. 81-91, 発行日 1990-01-01 |
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| ISSN | ||||||||||||||||||
| 収録物識別子タイプ | ISSN | |||||||||||||||||
| 収録物識別子 | 09162054 | |||||||||||||||||
| 抄録 | ||||||||||||||||||
| 内容記述タイプ | Abstract | |||||||||||||||||
| 内容記述 | [Abstract] The root mean square scattering angle and the scattering behaviors of the cosmic ray muous after traversing deep underground are extensively studied by considering various energy loss modes; ionization loss, electron pair production, bremsstrahlung, and nuclear interaction. The rms angular dependences are studied as functions of incident muon energies a.t sea level and observed muon energies in underground detector at various depths. As the extreme case of the calculations, we can get Rossi & Greisen expression and Eyges expression which have been very familiar to cosmic ray field. The rms angle of scatterings of muons is almost determined by the minimum energy of muons which is able to penetrate rock overburden an underground detector. The calculated results are compared with the broad deflected angular spreads of muons from Cygnus X-3 which have been observed by Soudan detector at a depth of 1800 hg/cm^2 and Nusex detector at a depth of 5000 hg/cm2. Also, we compare and discuss our calculated root mean square angles of (θ^2)^<-1/2> scatterings of low energy electrons with the measured values of electrons in the energy region of 5 MeV-40 MeV from the neutrino burst of SN 1987A which have been done by Kamiokande and IMB groups. | |||||||||||||||||
| フォーマット | ||||||||||||||||||
| 内容記述タイプ | Other | |||||||||||||||||
| 内容記述 | application/pdf | |||||||||||||||||
