在大星系团中,自我相似的能量
Francesco Miniati1, Andrey Beresnyak2
1Physics Department, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich, Switzerland.
Nature
|July 3, 2015
概括
星系团在热,流和磁组成之间保持着稳定的能量层次. 这种自相似的结构揭示了在宇宙结构形成过程中将引力能量转化为流的恒定效率.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 等离子体物理学的物理学
背景情况:
- 大规模的星系团包含热,动荡和磁化的集群内部介质.
- 星系团通过超音速流的积累成长,产生冲击和动荡.
- 能量从引力转化为动力,热,流和磁形式的能量转化尚未完全理解.
研究的目的:
- 调查集群内部介质中的能量转换模式.
- 为了确定星系团形成过程中能量转换的调节.
- 在宇宙学结构形成中识别自我相似性.
主要方法:
- 利用宇宙结构形成的计算模型.
- 分析了集群内部介质的能量组成部分 (热,,磁).
- 研究了从引力能量释放中产生流的效率.
主要成果:
- 在集群内部介质中发现了一个永久的能量层次结构.
- 观察到热,流和磁能密度的一致比率.
- 发现在积累过程中从引力能量中产生流的效率大约是恒定的.
结论:
- 星系团中的能量成分遵循一个稳定的,自我相似的层次结构.
- 这种层次结构反映了宇宙结构增长期间在流生成的恒定效率.
- 这些发现提供了关于星系团内的流加热和动纳摩作用的见解.
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