从聚合中子星二进制系统中重新连接驱动的快速无线电过渡
Elias R Most1,2,3, Alexander A Philippov4
1Princeton Center for Theoretical Science, Princeton University, Princeton, New Jersey 08544, USA.
Physical review letters
|June 30, 2023
概括
双中子恒星的合并可能会在碰撞之前产生快速的无线电爆发. 模拟显示了它们共享的磁层中的连贯发射机制,这可能解释了引力波事件的电磁对应物.
科学领域:
- 天体物理学 天体物理学
- 计算物理 计算物理
- 电磁主义 电磁主义
背景情况:
- 在中子星合并之前的电磁对应物的存在和机制在天体物理学中仍然是一个开放的问题.
- 了解这些现象对于多信使天文学和测试广义相对论至关重要.
研究的目的:
- 调查二进制中子星系统在它们合并之前产生的电磁对应物的可能性.
- 确定负责从这些系统产生短暂无线电辐射的物理机制.
主要方法:
- 全球无力电动力学模拟被用来建模双中子恒星磁层的行为.
- 分析的重点是确定共同的磁层内的连贯的发射过程.
主要成果:
- 模拟表明,具有亚磁性磁场的二进制中子星可以产生数毫秒快速的无线电爆发类型的短暂物.
- 确定了在合并之前在共享磁层中运行的特定的连贯发射机制.
结论:
- 该研究提供了一种可行的机制,用于在最终事件之前从中子星合并中生成可观测的电磁信号.
- 预测的发射频率为1011G的表面磁场的1020GHz范围,为未来的观测提供可测试的预测.
相关概念视频
Atomic Nuclei: Larmor Precession Frequency
1.5K
The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession,...
1.5K
Nuclear Fusion
22.6K
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
22.6K
Atomic Nuclei: Nuclear Relaxation Processes
683
In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis, the precessing magnetic moments are randomly oriented around the z-axis.
683
Atomic Nuclei: Types of Nuclear Relaxation
329
Nuclear relaxation restores the equilibrium population imbalance and can occur via spin–lattice or spin–spin mechanisms, which are first-order exponential decay processes.
In spin–lattice or longitudinal relaxation, the excited spins exchange energy with the surrounding lattice as they return to the lower energy level. Among several mechanisms that contribute to spin–lattice relaxation, magnetic dipolar interactions are significant. Here, the excited nucleus transfers...
In spin–lattice or longitudinal relaxation, the excited spins exchange energy with the surrounding lattice as they return to the lower energy level. Among several mechanisms that contribute to spin–lattice relaxation, magnetic dipolar interactions are significant. Here, the excited nucleus transfers...
329
Atomic Nuclei: Magnetic Resonance
689
The number of nuclear spins aligned in the lower energy state is slightly greater than those in the higher energy state. In the presence of an external magnetic field, as the spins precess at the Larmor frequency, the excess population results in a net magnetization oriented along the z axis. When a pulse or a short burst of radio waves at the Larmor frequency is applied along the x axis, the coupling of frequencies causes resonance and flips the nuclear spins of the excess population from the...
689
Nuclear Fission
9.8K
Many heavier elements with smaller binding energies per nucleon can decompose into more stable elements that have intermediate mass numbers and larger binding energies per nucleon—that is, mass numbers and binding energies per nucleon that are closer to the “peak” of the binding energy graph near 56. Sometimes neutrons are also produced. This decomposition of a large nucleus into smaller pieces is called fission. The breaking is rather random with the formation of a large...
9.8K


