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Extension of the cosmic-ray energy spectrum beyond the predicted Greisen-Zatsepin-Kuz'min cutoff
https://sucra.repo.nii.ac.jp/records/13313
https://sucra.repo.nii.ac.jp/records/13313d230f0dc-aebc-4c10-96a5-e8462ff8e3d5
名前 / ファイル | ライセンス | アクション |
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A1002755.pdf (93.7 kB)
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2008-08-19 | |||||
タイトル | ||||||
タイトル | Extension of the cosmic-ray energy spectrum beyond the predicted Greisen-Zatsepin-Kuz'min cutoff | |||||
言語 | ||||||
言語 | eng | |||||
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 | journal article | |||||
著者 |
Takeda, M
× Takeda, M× Hayashida, N× Honda, K× 井上, 直也× Kadota, K× Kakimoto, F× Kamata, K× Kawaguchi, S× Kawasaki, Y× Kawasumi, N× Kitamura, H× Kusano, E× Matsubara, Y× Murakami, K× Nagano, M× Nishikawa, D× Ohoka, H× Sakaki, N× Sasaki, H× Shinozaki, K× Souma, N× Teshima, M× Torii, R× Tsushima, I× Uchihori, Y× Yamamoto, T× Yoshida, S× Yoshii, H |
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著者 ローマ字 | ||||||
Takeda, M | ||||||
著者 ローマ字 | ||||||
Hayashida, N | ||||||
著者 ローマ字 | ||||||
Honda, K | ||||||
著者 ローマ字 | ||||||
Inoue, N | ||||||
著者 ローマ字 | ||||||
Kadota, K | ||||||
著者 ローマ字 | ||||||
Kakimoto, F | ||||||
著者 ローマ字 | ||||||
Kamata, K | ||||||
著者 ローマ字 | ||||||
Kawaguchi, S | ||||||
著者 ローマ字 | ||||||
Kawasaki, Y | ||||||
著者 ローマ字 | ||||||
Kawasumi, N | ||||||
著者 ローマ字 | ||||||
Kitamura, H | ||||||
著者 ローマ字 | ||||||
Kusano, E | ||||||
著者 ローマ字 | ||||||
Matsubara, Y | ||||||
著者 ローマ字 | ||||||
Murakami, K | ||||||
著者 ローマ字 | ||||||
Nagano, M | ||||||
著者 ローマ字 | ||||||
Nishikawa, D | ||||||
著者 ローマ字 | ||||||
Ohoka, H | ||||||
著者 ローマ字 | ||||||
Sakaki, N | ||||||
著者 ローマ字 | ||||||
Sasaki, H | ||||||
著者 ローマ字 | ||||||
Shinozaki, K | ||||||
著者 ローマ字 | ||||||
Souma, N | ||||||
著者 ローマ字 | ||||||
Teshima, M | ||||||
著者 ローマ字 | ||||||
Torii, R | ||||||
著者 ローマ字 | ||||||
Tsushima, I | ||||||
著者 ローマ字 | ||||||
Uchihori, Y | ||||||
著者 ローマ字 | ||||||
Yamamoto, T | ||||||
著者 ローマ字 | ||||||
Yoshida, S | ||||||
著者 ローマ字 | ||||||
Yoshii, H | ||||||
著者 所属 | ||||||
著者 所属 | ||||||
著者 所属 | ||||||
著者 所属 | ||||||
埼玉大学大学院理工学研究科物質科学部門 | ||||||
著者 所属(別言語) | ||||||
著者 所属(別言語) | ||||||
著者 所属(別言語) | ||||||
著者 所属(別言語) | ||||||
Graduate School of Science and Engineering, Saitama University | ||||||
書誌情報 |
PHYSICAL REVIEW LETTERS 巻 81, 号 6, p. 1163-1166, 発行日 1998 |
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年月次 | ||||||
1998-8 | ||||||
出版者名 | ||||||
出版者 | American Physical Society | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 00319007 | |||||
DOI | ||||||
関連タイプ | isIdenticalTo | |||||
識別子タイプ | DOI | |||||
関連識別子 | info:doi/10.1103/PhysRevLett.81.1163 | |||||
関連サイト | ||||||
内容記述タイプ | Other | |||||
内容記述 | http://link.aps.org/abstract/PRL/v81/p1163 | http://link.aps.org/abstract/PRL/v81/p1163 | |||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | The cosmic-ray energy spectrum above 10(18).5 eV is reported using the updated data set of the Akeno Giant Air Shower Array from February 1990 to October 1997. The energy spectrum extends beyond 10(20) eV and the energy gap between the highest energy event and the others is being filled up with recently observed events. The spectral shape suggests the absence of the 2.7 K cutoff in the energy spectrum or a possible presence of a new component beyond the 2.7 K cutoff. [S0031-9007(98)06893-8]. | |||||
版 | ||||||
[出版社版] | ||||||
著者版フラグ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
資源タイプ | ||||||
内容記述タイプ | Other | |||||
内容記述 | text | |||||
フォーマット | ||||||
内容記述タイプ | Other | |||||
内容記述 | application/pdf | |||||
作成日 | ||||||
日付 | 2008-08-20 | |||||
日付タイプ | Created | |||||
アイテムID | ||||||
A1002755 |