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中子星中中子子反中子转换的影响
Itzhak Goldman1,2, Rabindra N Mohapatra3, Shmuel Nussinov2
1Afeka College, Department of Physics, 6998812 Tel Aviv, Israel.
Physical review letters
|February 21, 2025
概括
中子星中中子-反中子过渡对冷却,旋转和双脉冲星轨道周期的影响可以忽略不计. 我们的分析证实,这些天体物理现象是微不足道的.
科学领域:
- 天体物理学 天体物理学
- 粒子物理学 粒子物理学
背景情况:
- 中子星是极端的天体物理物体.
- 中子-反中子转换是假设的过程.
研究的目的:
- 为了研究中子-反中子转换对中子星特性的影响.
- 量化对冷却,旋转和二进制脉冲星轨道演变的影响.
主要方法:
- 在中子星内部中子-反中子过渡的理论建模.
- 对冷却速度的天体物理计算.
- 对旋转动态的分析.
- 对二进制脉冲星系统的建模.
主要成果:
- 中子-反中子转换对中子星冷却产生微不足道的影响.
- 发现对中子星旋转速率的影响是微不足道的.
- 由于这些转变,对二进制脉冲星的轨道周期的预测增加是微不足道的小.
结论:
- 中子-反中子过渡不会显著改变中子星的可观测性质.
- 目前对中子星的天体物理学观测不太可能受到中子-反中子过渡的影响.
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