论文标题
磁性连接
The Magnetar Connection
论文作者
论文摘要
我们研究了已知磁场和高磁场的偶极表面磁场（b $ _ {s} $）和旋转period（p $ _s $）（b $ _s $ $ $ $ \ gtrsim 10^{13} $ 〜g）无线电脉冲脉冲的组合演变（b $ _s $ _S $ _s $ _s $ _s $ _s $ _s $ _s $ \ gtrsim 10^{13} $ g）。我们研究了这些物体的长期行为，假设对磁场的欧姆耗散简单。确定这些中子星可能会进入的区域（在p $ _s $ -b $ _s $ plane中），在越过死亡线进入Pulsar Graveyard之前，我们会评论磁场与其他类别的中子星之间的可能联系。
We investigate the combined evolution of the dipolar surface magnetic field (B$_{s}$) and the spin-period (P$_s$) of known magnetars and high magnetic field (B$_s$ $ \gtrsim 10^{13}$~G) radio pulsars. We study the long term behaviour of these objects assuming a simple ohmic dissipation of the magnetic field. Identifying the regions (in the P$_s$-B$_s$ plane) in which these neutron stars would likely move into, before crossing the death-line to enter the pulsar graveyard, we comment upon the possible connection between the magnetars and other classes of neutron stars.
