论文标题
关于长伽玛射线爆发余辉的起源，作为二进制驱动型高诺沃的同步辐射
On the Origin of the Long Gamma-Ray Burst Afterglow as Synchrotron Radiation from Binary-Driven Hypernovae
论文作者
论文摘要
长伽马射线爆发显示出X射线，光学和无线电波长的余辉发射，其发光度随时间而逐渐淡化，并且几乎相同的幂律行为。在本次演讲中，我提出了一种分析治疗，表明这种余辉是由与二进制驱动的高诺伏那维相关的超新星喷射的同步辐射产生的。
Long gamma-ray bursts show an afterglow emission in the X-rays, optical, and radio wavelengths with luminosities that fade with time with a nearly identical power-law behavior. In this talk, I present an analytic treatment that shows that this afterglow is produced by synchrotron radiation from the supernova ejecta associated with binary-driven hypernovae.
