论文标题
在等离子体存在的情况下，从轴恒星中子恒星二进制轴线辐射，倾斜旋转轴
Radiation from Axion star-Neutron star binaries with a tilted rotation axis in the presence of plasma
论文作者
论文摘要
我们使用Axion Star的$ f（r）= \ text {sech（r/r）} $配置文件研究了由轴恒星中心二进制二进制二进制二进制辐射的形式。我们的分析考虑了中子星的共旋转等离子体。我们发现，与垂直的情况相比，如果中子恒星的旋转向轴突恒星中性星轨道的平面倾斜，则辐射功率有明显的增强。我们还检查了中子恒星的共旋转等离子体是否可以在发射的能力中起作用，我们发现，即使稀轴恒星原则上可以比密集的轴突恒星更有效地辐射，但它们将被中子星的潮汐力拉开
We investigate the form of the radiation emitted by an axion star-neutron star binary using a $f(r)=\text{sech(r/R)}$ profile for the axion star. Our analysis takes into account the co-rotating plasma of the neutron star. We find that that there is significant enhancement to the radiated power if the neutron star's spin is tilted towards the plane of the axion star-neutron star orbit, compared to the case where it is perpendicular. We also examine whether the neutron star's co-rotating plasma can play a role in the emitted power and we find that even though dilute axion stars can in principle radiate more efficiently than dense axion stars, they will be pulled apart by the tidal forces of the neutron star
