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Updated: Feb 17, 2026

Setting Limits on Supersymmetry Using Simplified Models
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Published on: November 15, 2013

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ニュートリノ質量階層の発見のための大気中ニュートリノ振動のシミュレーション

Mourad Fouka1, Sami Slimateni1,2

  • 1Division of Stellar and High Energy Astrophysics, Center of Research in Astronomy, Astrophysics and Geophysics (CRAAG), B.P. 63, Route de l'Observatoire, Bouzareah, 16340, Algeries, Algeria.

Radiation protection dosimetry
|February 16, 2026
PubMed
まとめ

シミュレーションでは,3-10 GeVのエネルギー範囲が中性子の質量階層を決定するのに有望であることを示しています. この研究は,地球を通る大気中のニュートリノ振動をモデル化するためにPHASTコードを使用しました.

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