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Comments on a Solar Neutrino Flux of the Kamiokande Observation
https://kindai.repo.nii.ac.jp/records/11243
https://kindai.repo.nii.ac.jp/records/11243f06f5590-5cbe-4380-8301-744e94b3b371
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
AN10074306-19940130-0043.pdf (492.5 kB)
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| Item type | ☆紀要論文 / Departmental Bulletin Paper(1) | |||||||||||||||||
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| 公開日 | 2015-03-19 | |||||||||||||||||
| タイトル | ||||||||||||||||||
| タイトル | Comments on a Solar Neutrino Flux of the Kamiokande Observation | |||||||||||||||||
| 言語 | en | |||||||||||||||||
| 著者 |
Kitamura, T.
× Kitamura, T.
× Nakatsuka, T.
× Konishi, T.
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| 言語 | ||||||||||||||||||
| 言語 | eng | |||||||||||||||||
| キーワード | ||||||||||||||||||
| 主題 | 96.60.K_x Solar interior (including neutrino problem), 03.80.+r General theory of scattering | |||||||||||||||||
| 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, T. | |||||||||||||||||
| 著者(英) | ||||||||||||||||||
| 言語 | en | |||||||||||||||||
| 値 | Nakatsuka, T. | |||||||||||||||||
| 著者(英) | ||||||||||||||||||
| 言語 | en | |||||||||||||||||
| 値 | Konishi, T. | |||||||||||||||||
| 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 | Department of Mathematics and Physics, Kinki 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 | 近畿大学 | |||||||||||||||||
| 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 6, p. 43-51, 発行日 1994-01-01 |
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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] Results of solar neutrino observations by the Kamiokande (ν_ee→ν_ee Experiment), Chlorine and Gallium Experiments are in apparent disagreement among them. However, it is necessary to consider possible errors before making such a judgement. We have comments on the Kamiokande II results to point out as followings; (1) in the Kamiokande II paper there seems a serious disconsistency in the expected event rate of the Standard Solar Model(SSM) calculation between their used value in derivations of the data/SSM and their calculated value due to the Bahcall and Ulrich theory. Using the correct expected value for the SSM, we obtain a value of 0.35 for the data/the SSM in a place of 0.46. (2) The Kamiokande group has concluded that the observed cos 0 distribution of collimated γ rays with the Ni(n,γ)Ni^* source endorses the proper procedure of Monte Carlo simulations using the EGS4 code for angular distributions in the reaction of ν_ee→ν_ee. However, Smirnov-Cramer-Von Mieses test for the goodness-of-fit gives a poor significance probability of less than 0.001. (3) Using more adequate scattering formulae instead of EGS4 code which is used in the Kamiokande analysis, we can show 0.31 ± 0.14 for the data/the SSM with Mott formula and 0.33 ± 0.14 for Williams formula to the Kamiokande II data. | |||||||||||||||||
| フォーマット | ||||||||||||||||||
| 内容記述タイプ | Other | |||||||||||||||||
| 内容記述 | application/pdf | |||||||||||||||||
