论文标题
在参与磁力中心的粒子的比例上
On the fraction of particles involved in magneto-centrifugally generated ultra-high energy electrons in the Crab pulsar
论文作者
论文摘要
图表列出了在PULSAR大气中产生的超高能电子（$ \ sim 600 $ tev）的地球旅程，这是通过图表的磁磁性降低的landau阻尼的landau抑制了原主电子上的langmuir波（旋转速度的旋转减速）。结果表明，就像它们逃脱光缸区域一样，超高的能量颗粒与蟹状的介质相互作用，通过量子同步器工艺迅速失去了能量，产生了高能的伽玛射线〜$ \ sim 0.6 $ pev。与星际介质中的宇宙背景辐射相互作用，仅这些超高能量光子（通过$γγ$通道）仅一小部分，然后转换为电子峰值对。这些光子的检测通量对参与超高能光子生成过程的磁层颗粒的分数（$ 4 \ times 10^{ - 7} $）施加了上限（$ 600 $ $ 600 $ TEV）。
The earthward journey of ultra high energy electrons ($\sim 600$ TeV) produced in the Pulsar atmosphere by Landau damping of magneto-centrifugally excited Langmuir waves (drawing energy form the rotational slowdown) on primary electrons, is charted. It is shown, that just as they escape the light cylinder zone, the ultra-high energy particles, interacting with the medium of the Crab nebula, rapidly loose their energy via the quantum synchrotron process, producing highly energetic gamma rays ~ $\sim 0.6$PeV. Interacting with the cosmic background radiation in the interstellar medium, only a tiny fraction of these ultra high energy photons (via the $γγ$ channel) are, then transformed into electron-positron pairs. Detected flux of these photons imposes an upper limit on the fraction ($4\times 10^{-7}$) of the magnetospheric particles involved in the process of generation of ultra-high energy photons (up to $600$ TeV).
