论文标题
微量夸张M33 x-7的喷射喷气机中的高能量中微子和伽马射线排放
High energy neutrino and gamma-ray emission in the jets of the microquasar M33 X-7
论文作者
论文摘要
在这项工作中，在通过研究精心拟研究的SS 433银河微QuaSar测试了算法的可靠性后，我们专注于中微子和$γ$ ray-ray-ray-ray-ray-ray-ray-ray-ray ragagalactic M33 x-7系统。这是一个最近发现的X射线二进制系统，位于相邻的Galaxy Messier 33中，尚未详细建模。在我们方法的背景下，由M33 X-7的磁化天体物理喷气产生的中微子和$γ$ - 射线的能光谱在我们方法的背景下产生，源自衰减（和散射）过程，在产生的二次颗粒中发生，假设首先是热（相对论）散布在热（p-p-p-p-p-p-p-p的互动）上（p-p-p-p-p-p-p-p-p-p-p-p-p-P-P互动机械）。
In this work, after testing the reliability of our algorithms through numerical simulations on the well-studied SS 433 Galactic microquasar, we focus on neutrino and $γ$-ray emissions from the extragalactic M33 X-7 system. This is a recently discovered X-ray binary system located in the neighbouring galaxy Messier 33 which has not yet been modelled in detail. The neutrino and $γ$-ray energy spectra, produced from the magnetized astrophysical jet of M33 X-7, in the context of our method are assumed to originate from the decay (and scattering) processes taking place among the secondary particles produced assuming that, first, hot (relativistic) protons of the jet scatter on thermal ones (p-p interaction mechanism).
