http://arxiv.org/abs/2012.08767
The gluon condensation predicted by a nonlinear QCD evolution equation can naturally explain the typical broken power law in the $\gamma$-ray spectra at very high energy. This result is used to perfect the incomplete spectra HESSs J1826-130, J1641-463 and J1741-302. We show the distinctive characteristics of these spectra, which are different from the other spectra models and they can be tested by further observations.
J. Ruan, Z. Zheng and W. Zhu
Thu, 17 Dec 20
8/85
Comments: 21pages, 9figures
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