初期の宇宙における音響振動と今日の音響振動
C J Miller1, R C Nichol, D J Batuski
1Department of Physics, Carnegie Mellon University, Pittsburgh, PA 15213, USA.
まとめ
科学者たちは,宇宙マイクロ波背景 (CMB) と物質の分布における音響振動を検出しました. 異なる宇宙時間におけるこれらの発見は,ホット・ビッグバンモデルを支持する.
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
- 素粒子物理学 素粒子物理学について
背景:
- 初期の宇宙は,光子と物質が結合した熱い,イオン化されたプラズマでした.
- 重力崩壊と光子圧力は,この原始的な流体の中で音響的振動を生み出しました.
研究 の 目的:
- 宇宙マイクロ波背景 (CMB) で検出された音響振動を,現在の物質密度分布の振動と比較する.
- 標準的なホットビッグバンモデルに対するさらなる証拠を提供するために.
主な方法:
- BOOMERANGとMAXIMAのCMBデータ (赤色偏移 ~1000) を分析した.
- 物質密度電力スペクトルデータとの比較 (レッドシフト ~0.1).
主要な成果:
- CMBにおける音響振動の検出. CMBにおける音響振動の検出.
- 物質密度電力スペクトルの対応する振動の一貫した検出.
- CMBと物質分布観測の間の合意.
結論:
- 2つの異なる宇宙学時代の一貫した結果は,標準的なホットビッグバンモデルを強く支持しています.
- 音響振動は,初期の宇宙の物理学の予測可能な印として機能します.
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