论文标题
中子恒星磁层中的超线移动电流板对辐射的启发式描述
A heuristic account of the radiation by the superluminally moving current sheet in the magnetosphere of a neutron star
论文作者
论文摘要
在Ardavan（2021年，{\ it Mnras}，{\ bf 507}，4530）中呈现的中子恒星磁层中的辐射的数学处理结果，在这里在这里有更多透明的物理术语来解释。这些结果不仅为从脉冲星（其亮度温度，极化，频谱，具有微观结构的亮度温度，极化，频谱，剖面以及无线电和伽马射线峰之间的相位滞后，以及在无线电和伽玛的能量需求之间的差异）之间的差异，但它们在无线电和γ-射线的范围之间的差异之间的差异，不仅提供了一个无所不包的解释。爆发和伽马射线爆发。
Results of the mathematical treatment of the radiation by the superluminally moving current sheet in the magnetosphere of a neutron star, which was presented in Ardavan (2021, {\it MNRAS}, {\bf 507}, 4530), are explained here in more transparent physical terms with the aid of illustrations. Not only do these results provide an all-encompassing explanation for the salient features of the radiation received from pulsars (its brightness temperature, polarization, spectrum, profile with microstructure and with a phase lag between the radio and gamma-ray peaks, and the discrepancy between the energetic requirements of its radio and gamma-ray components), but they also shed light on the putative energetic requirements of magnetars and the sources of fast radio bursts and gamma-ray bursts.
