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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...
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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.
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A neutral atom consists of a positively charged nucleus surrounded by a negatively charged electron cloud. When placed in an external electric field, the external electric force pulls the electrons and nucleus apart, opposite to the intrinsic attraction between the nucleus and the electrons. The opposing forces balance each other with a slight shift between the center of masses of the nucleus and the electron cloud, resulting in a polarized atom. On the other hand, a few molecules, like water,...
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Hyperpolarized Xenon for NMR and MRI Applications
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来自磁星的极化X射线

Roberto Taverna1, Roberto Turolla1,2, Fabio Muleri3

  • 1Department of Physics and Astronomy, University of Padova, I-35131 Padova, Italy.

Science (New York, N.Y.)
|November 10, 2022
PubMed
概括
此摘要是机器生成的。

极化X射线观测显示磁星4U 0142+61具有复杂的磁场. 极化随能量变化而变化,这表明磁星的磁层中的辐射分散.

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科学领域:

  • 天体物理学
  • 高能天体物理学
  • 中子星研究

背景情况:

  • 磁星是具有极强磁场的中子星.
  • 对于研究磁星特性而言,X射线观测至关重要.
  • 极化测量提供了对磁场和表面特征的洞察.

研究的目的:

  • 为了研究磁星4U 0142+61发出的X射线的极化.
  • 为了确定X射线偏振的程度和能量依赖性,
  • 测试磁性发射机制的模型.

主要方法:

  • 使用成像X射线极度测量探测器 (IXPE) 进行观测.
  • 从4U 0142+61测量了X射线的线性极化度和角度.
  • 在2~8千电子伏特能量范围内分析极化.

主要成果:

  • 检测到 13.5 ± 0.8% 的显著线性极化度,平均为 2- 8 keV.
  • 观察到的能量依赖偏振:15.0 ± 1.0% (2-4 keV),低偏振 (~4-5 keV) 和35.2 ± 7.1% (5.5-8 keV).
  • 记录了90°偏振角度转移在4-5keV.

结论:

  • 观察到的极化特性与热表面辐射一致.
  • 在磁星的磁层中散射带电粒子可能会重新处理辐射.
  • 这些发现支持涉及磁层粒子相互作用的模型.