相关实验视频
Updated: Aug 20, 2025

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
10.4K
极化雷射暗示粒子在冲击中的加速
Ioannis Liodakis1, Alan P Marscher2, Iván Agudo3
1Finnish Centre for Astronomy with ESO, FI-20014, University of Turku, Turku, Finland. yannis.liodakis@utu.fi.
Nature
|November 23, 2022
概括
研究人员检测到来自Blazar Markarian 501的X射线极化, 显示出比光学光更高的极化. 这一发现表明冲击阵线在活跃的星系核中加速粒子.
科学领域:
- 天体物理学
- 高能天体物理学
- 血物理
背景情况:
- 耀星是活跃的星系核,其喷射由高能粒子 (高达1 TeV) 产生的光.
- 在由超大质量黑洞驱动的布拉撒喷流中, 粒子加速的机制在很大程度上是未知的.
- 之前的极化测量 (从无线电到光学) 探测了遥远的区域,而不是粒子加速地点.
研究的目的:
- 通过测量X射线极化来研究布拉撒射线中的粒子加速机制.
- 探索磁场在高能粒子加速中的作用.
- 在喷气中探测离粒子加速位置更近的条件.
主要方法:
- 检测到来自马卡里安501 (Mrk 501) 的X射线极化.
- 测量X射线线性极化度 (ΠX) 和极化角度.
- 与现有的光学和无线电偏振数据进行X射线偏振测量的比较.
主要成果:
- 来自Mrk 501的显著X射线线性极化 (ΠX ≈10%) 的检测.
- 测量的X射线极化度大约是光学波长观察到的值的两倍.
- 发现X射线极化角度与无线射线方向平行.
结论:
- 这些结果强烈地表明, 布拉撒射流中的冲击阵线是粒子加速的主要地点.
- 波长增加的极化意味着与冲击距离的增加等离子体流.
- 通过X射线极化测量,可以直接探测到Blazar喷射中的粒子加速过程.
相关概念视频
Potential Due to a Polarized Object
459
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,...
459
Momentum And Radiation Pressure
2.1K
An object absorbing an electromagnetic wave would experience a force in the direction of propagation of the wave. This force occurs because electromagnetic waves contain and transport momentum. The force accounts for the wave's radiation pressure exerted on the object. Maxwell's prediction was confirmed in 1903 by Nichols and Hull by precisely measuring radiation pressures with a torsion balance. The measuring instrument had mirrors suspended from a fiber kept inside a glass container.
2.1K
Shock Waves
2.1K
While deriving the Doppler formula for the observed frequency of a sound wave, it is assumed that the speed of sound in the medium is greater than the source's speed through it. When this condition is breached, a shock wave occurs.
When the source's speed approaches the speed of sound, constructive interference between successive wavefronts emitted by the source occurs immediately behind it. Initially, scientists believed that this constructive interference would result in such high...
When the source's speed approaches the speed of sound, constructive interference between successive wavefronts emitted by the source occurs immediately behind it. Initially, scientists believed that this constructive interference would result in such high...
2.1K
The de Broglie Wavelength
26.1K
In the macroscopic world, objects that are large enough to be seen by the naked eye follow the rules of classical physics. A billiard ball moving on a table will behave like a particle; it will continue traveling in a straight line unless it collides with another ball, or it is acted on by some other force, such as friction. The ball has a well-defined position and velocity or well-defined momentum, p = mv, which is defined by mass m and velocity v at any given moment. This is the typical...
26.1K
Motion Of A Charged Particle In A Magnetic Field
5.1K
A charged particle experiences a force when moving through a magnetic field. Consider the field to be uniform and the charged particle to move perpendicular to it. If the field is in a vacuum, the magnetic field is the dominant factor determining the motion. Since the magnetic force is perpendicular to the direction of motion, a charged particle follows a curved path. The particle continues to follow this curved path until it forms a complete circle. Another way to look at this is that the...
5.1K
Atomic Nuclei: Nuclear Relaxation Processes
701
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.
701

