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Updated: Jul 8, 2026

09:41
Blast Quantification Using Hopkinson Pressure Bars
Published on: July 5, 2016
まとめ
ハッブル定数は,宇宙の膨張速度を測定する. 現在の測定は大きく異なるため,宇宙学的モデルや理論との矛盾が生じます.
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
背景:
- ハッブル定数 (H0) は,宇宙の膨張速度を定量化し,宇宙のスケールと年齢を決定するのに不可欠です.
- 正確なH0測定は,宇宙学的モデルを検証し,宇宙の進化を理解するために不可欠です.
研究 の 目的:
- ハッブル定数の決定における継続的な課題と不一致を強調するために.
- 異なるH0値が宇宙論理論に及ぼす影響について議論する.
主な方法:
- 銀河の衰退速度と距離の測定は,H0.0を決定するために使用されます.
- 正確な銀河距離測定のための新しい技術の開発は進行中です.
主要な成果:
- 現在のH0の決定は,幅広く,ほぼ2の因数で示されています.
- 局所的な測定はしばしばより高いH0値を出し,いくつかの理論的予測と矛盾する.
結論:
- 継続的な校正の不確実性と,体系的なエラーが,H0の決定的な値の実現を妨げています.
- 地元と世界のH0測定値の差異は,現在の宇宙学的な理解と構造形成と恒星の進化の理論に重大な課題をもたらします.
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