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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
欠落しているバリオンと,温かい熱い銀河間媒質
Fabrizio Nicastro1, Smita Mathur, Martin Elvis
1Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA. fnicastro@cfa.harvard.edu
まとめ
宇宙学者は,暖かい熱い銀河間媒質にあると考えられている,行方不明のバリオンを探しています. これらの難解な宇宙の成分を見つけることは,私たちの宇宙の理解を検証する鍵です.
科学分野:
- コスモロジー・コスモロジーとは
- 天体物理学 天体物理学
- 銀河間媒介は銀河間媒介である.
背景:
- 観測可能な宇宙には,予想されるバリオン物質の半分しか含まれていない.
- ほとんどのバリオンは,温かい熱い銀河間媒介 (WHIM) に存在すると仮定されています.
- この欠落した物質は,宇宙構造の形成の間に衝撃で加熱されたと考えられています.
研究 の 目的:
- 宇宙に欠けているバリオンを見つけ出すために.
- バリオン物質の完全な在庫を作成するために.
- 標準宇宙学モデルをテストするために.
主な方法:
- 観測天文学は,観測による天文学である.
- コスモロジック・シミュレーション
- 銀河間ガス特性の分析
主要な成果:
- この研究は,欠落しているバリオンの理論的分布に焦点を当てています.
- 温かい熱い銀河間媒体の期待される性質を強調しています.
- それは,観察的証拠の必要性を強調しています.
結論:
- 欠落しているバリオンの存在と分布を確認することは極めて重要です.
- この研究は,標準宇宙論モデルの検証に影響を与えます.
- 温かい熱い銀河間媒体を検出するには,さらなる観測努力が必要です.
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