论文标题
正交脉冲星作为脉冲星的关键测试
Orthogonal pulsars as a key test for pulsar evolution
论文作者
论文摘要
目前，尚无有关无线电脉冲星中磁性轴和旋转轴之间倾斜角$χ$演变的直接信息。至于脉冲星进化的理论模型，它们既预测对齐的倾斜角度$χ$至$ 0^{\ circ} $的进化，及其对抗及其对准，即演变为$ 90^{\ circ} $。在本文中，我们证明了插入式脉冲星的统计数据可以为我们提供关键测试，以解决对齐/反平衡问题作为正交插入式脉冲星的数量（$χ\ 90^{\ circ} $）极大地取决于进化轨迹。
At present, there is no direct information about the evolution of inclination angle $χ$ between magnetic and rotational axes in radio pulsars. As to theoretical models of pulsar evolution, they predict both the alignment, i.e. evolution of inclination angle $χ$ to $0^{\circ}$, and its counter-alignment, i.e. evolution to $90^{\circ}$. In this paper, we demonstrate that the statistics of interpulse pulsars can give us the key test to solve the alignment/counter-alignment problem as the number of orthogonal interpulse pulsars ($χ\approx 90^{\circ}$) drastically depends on the evolutionary trajectory.
