中子星中的短距离相关性和Urca过程
1<a href="https://ror.org/05vmv8m79">Frankfurt Institute for Advanced Studies</a>, D-60438 Frankfurt am Main, Germany and Institute of Theoretical Physics, <a href="https://ror.org/00yae6e25">University of Wroclaw</a>, 50-204 Wroclaw, Poland.
Physical review letters
|November 12, 2024
概括
紧恒星中的高动量中子-质子对挑战了费米液体理论. 纳入短距离相关性改变了乌尔卡星的过程速率,影响了关于紧恒星冷却的理论.
科学领域:
- 核物理 核物理 核物理
- 天体物理学 天体物理学
- 紧的恒星物理 紧的恒星物理
背景情况:
- 最近的JLab实验揭示了紧的恒星中的高动量中子-质子对.
- 这些发现与标准费米液体理论对中子-质子流体混合物的预测有所不同.
研究的目的:
- 为了研究非费尔米流体贡献对紧恒星中乌尔卡过程速度的影响.
- 分析短距离相关性如何影响质子光谱宽度和Urca过程.
主要方法:
- 计算Urca过程速度的计算.
- 包括从质子光谱宽度上的短距离相关性中产生的非费米流体效应.
主要成果:
- 在低温下,Urca过程速度显示出与费米液体预测的显著偏差.
- 在中子星中Urca过程的以前高值被质子分数的平稳增加所取代.
结论:
- 短距离的相关性显著改变了紧的恒星中的Urca过程.
- 这些修改可能对理解紧恒星冷却机制产生重大影响.
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