论文标题
旋转磁化恒星中带电颗粒的加速度
Acceleration of charged particles in rotating magnetized star
论文作者
论文摘要
由于磁化恒星的旋转，可能会驱逐紧凑型恒星的带电颗粒并加速电场。对于中子或杂化恒星，带负电荷的颗粒通常是电子，正带正电荷的颗粒主要是质子和铁。而奇怪的恒星的存在也包括从恒星表面弹出陌生人的可能性。从所有已知的脉冲星中发出的这种陌生人的通量在$ 10^9-10^{10} $ gev的范围内。因此，这种巨大的陌生人可以成为仍然避开我们的最高能源宇宙射线来源的候选者之一。我们的模型提出了这些超高能宇宙射线的可能起源。
Charged particles at the crust of compact stars may be ejected and accelerated by the electric field generated due to the rotation of the magnetized star. For neutron or hybrid stars, the negatively charged particles are usually electrons, and the positively charged particles are mainly protons and Iron. Whereas the existence of strange stars also includes the possibility of ejection of strangelets from the star surface. The flux of such strangelets emitted from all known pulsars is in the range of $10^9-10^{10}$ GeV. Therefore, such massive strangelets can be one of the candidates for the sources of the highest-energy cosmic rays that have still eluded us. Our model proposes a possible origin of these ultra high energy cosmic rays.
