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Updated: Jun 8, 2025

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Hyperpolarized Xenon for NMR and MRI Applications
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脉冲星消灭和真空无线电发射来自Axion云
Andrea Caputo1, Samuel J Witte2,3, Alexander A Philippov4
1CERN, Department of Theoretical Physics, Esplanade des Particules 1, P.O. Box 1211, Geneva 23, Switzerland.
Physical review letters
|November 1, 2024
概括
在脉冲星极帽中可以形成一个由重力绑定的轴子组成的密集云. 这种动脉云可以间歇地屏蔽电场,导致脉冲星的无线电辐射周期性地变为零,或产生狭窄的无线电线.
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:
- 脉冲星是快速旋转的中子星,具有强大的磁场.
- 非相对论的轴子是假设的粒子,可以在极端的天体物理环境中产生.
研究的目的:
- 调查axion云和脉冲星磁层电动力学之间的相互作用.
- 确定动力云对脉冲星粒子加速和无线电辐射的影响.
主要方法:
- 轴心云形成的理论建模及其对脉冲星磁层的影响.
- 对动力场动态和电动力学选机制的分析.
主要成果:
- 光轴子 (m_a 10^-7 eV) 可以屏蔽电场,导致脉冲星无线电辐射的周期性取消.
- 较重的轴子可以导致不连贯的振荡,通过一种新的发射过程产生狭窄的无线电线.
结论:
- 轴云显著影响脉冲星发射机制,提供新的观测信号.
- 轴承云和脉冲星电动力学之间的相互作用为轴承物理提供了一个独特的探测器.
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