论文标题
螃蟹星云的高能量排放
High Energy emission from Crab Nebula
论文作者
论文摘要
已经观察到蟹状星云的耀斑发作。探索了一种新的排放机制。通过某些机制（在论文中描述的某些机制）将螃蟹脉冲星中的颗粒加速到多个TEV能量，这是观察到发射的原因。我们认为，在加速高能之后，它们可以保持无力度的状态 - 沿着磁场线移动，以至于没有力对其进行任何作用。这样，他们就可以毫无损失地搬到星云，这使得蟹状星云的TEV能量发射很可能。
Flaring episodes from Crab Nebula have been observed. A new mechanism of emission is explored. Particles in Crab pulsar are accelerated to multiple Tev energies, by some mechanisms, described in the paper and they are the reason of observed emission. We argue, that after accelerating to high energies, they may maintain the force-free regime - moving along the magnetic field lines in such a way that no force acts on them. This way, they can move to the Nebula without loss, which makes Tev energy emission from Crab Nebula quite possible.
