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Updated: Jul 17, 2026

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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
宇宙のサイクルモデルである
Paul J Steinhardt1, Neil Turok
1Joseph Henry Laboratories, Princeton University, Princeton, NJ 08544, USA. steinh@princeton.edu
まとめ
この宇宙論的モデルは,宇宙が"バン"と"クランチ"の終わりのないサイクルを持つことを提案しています. それぞれのサイクルには,ゆっくりと膨張と収縮が特徴であり,次の宇宙時代のための条件を提供します.
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
- 理論物理学の理論物理学
背景:
- 現在の宇宙学モデルは,宇宙の起源と進化を説明するのに苦労しています.
- 単一の始まりと終わりの概念は,循環的宇宙理論によって挑戦されています.
研究 の 目的:
- 周期的な宇宙を特徴とする新しい宇宙学的モデルを提案する.
- 宇宙の均質性,平らさ,そしてエネルギーをバング・クラッチのシーケンスを通して説明する.
主な方法:
- 宇宙時代の理論的モデリング.
- 宇宙サイクル間の移行期間の条件の分析.
主要な成果:
- 提案されたモデルは,宇宙の絶え間ない連続のパンクとクランチを記述しています.
- 有限の温度と密度は,バン・クランク・トランジションで維持されます.
- 各サイクルには,ゆっくりと加速された膨張に続いて収縮が含まれる.
結論:
- サイクルモデルは,インフレ宇宙論の代替案である.
- バング・クラッチのシーケンスによって,自然に次のサイクルに必要な均質性,平らさ,エネルギーが生成されます.
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