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  1. B100 理学部/理学研究科
  2. B100a 雑誌掲載論文
  3. 学術雑誌

OPERA -First Beam Results-

http://hdl.handle.net/2237/12011
http://hdl.handle.net/2237/12011
f4716fee-5f8b-4d97-b044-8519ff62fb8f
名前 / ファイル ライセンス アクション
31139451.pdf 31139451.pdf (729.2 kB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2009-08-03
タイトル
タイトル OPERA -First Beam Results-
言語 en
著者 NAKAMURA, M.

× NAKAMURA, M.

WEKO 30850

en NAKAMURA, M.

Search repository
アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
権利
言語 en
権利情報 Copyright (2008) American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.
キーワード
主題Scheme Other
主題 elementary particle physics
キーワード
主題Scheme Other
主題 neutrino oscillation
キーワード
主題Scheme Other
主題 nuclear emulsion
抄録
内容記述 OPERA is a long base-line neutrino oscillation experiment to detect tau-neutrino appearance and to prove that the origin of the atmospheric muon neutrino deficit observed by Kamiokande is the neutrino oscillation. A Hybrid emulsion detector, of which weight is about 1.3 kton, has been installed in Gran Sasso laboratory. New muon neutrino beam line, CNGS, has been constructed at CERN to send neutrinos to Gran Sasso, 730 km apart from CERN. In 2006, first neutrinos were sent from CERN to LNGS and were detected by the OPERA detector successfully as planned.
言語 en
内容記述タイプ Abstract
出版者
言語 en
出版者 American Institite of Physics
言語
言語 eng
資源タイプ
資源タイプresource http://purl.org/coar/resource_type/c_6501
タイプ journal article
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
DOI
関連タイプ isVersionOf
識別子タイプ DOI
関連識別子 https://doi.org/10.1063/1.2898957
ISSN
収録物識別子タイプ PISSN
収録物識別子 0094-243X
書誌情報 en : AIP Conference Proceedings

巻 981, 号 1, p. 26-28, 発行日 2008-02-21
フォーマット
application/pdf
著者版フラグ
値 publisher
URI
識別子 http://dx.doi.org/10.1063/1.2898957
識別子タイプ DOI
URI
識別子 http://hdl.handle.net/2237/12011
識別子タイプ HDL
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