论文标题
活性银核的光速变化
Light speed variation from active galactic nuclei
论文作者
论文摘要
最近对来自伽马射线爆发的高能量光子〜（GRB）的研究表明，轻速变化$ v（e）= c（1-e/e/e _ {\ mathrm {lv}}）$，带有$ e_ \ mathrm {lv} = 3.6 \ 3.6 \ times 10^{17} {17} $ GEV。我们从三个活性银河核（AGN）的光曲线上的先前观察结果，即Markarian 421（MRK 421），Markarian 501（MRK 501）和PKS 2155-304中检查了这种速度变化。我们表明，与这些AGN的光曲线相关的几种现象可以作为对GRBS确定的光速变化的支持。
Recent studies on the high-energy photons from gamma-ray bursts~(GRBs) suggested a light speed variation $v(E)=c(1-E/E_{\mathrm{LV}})$ with $E_\mathrm{LV}=3.6\times 10^{17}$ GeV. We check this speed variation from previous observations on light curves of three active galactic nuclei (AGNs), namely Markarian 421 (Mrk 421), Markarian 501 (Mrk 501) and PKS 2155-304. We show that several phenomena related to the light curves of these AGNs can serve as the supports for the light speed variation determined from GRBs.
