论文标题
合并中子星的电磁垂缘
Electromagnetic draping of merging neutron stars
论文作者
论文摘要
我们首先得出了一组描述相对论无力等离子体的一般固定构型的方程组，而无需假设任何几何对称性。然后，我们证明，合并中子恒星的电磁相互作用必然是耗散性的，这是由于电磁悬垂的影响 - 在恒星附近（在单磁化情况下）或在磁层边界（在双磁性情况下）的耗散区域的产生。我们的结果表明，即使在单个磁化情况下，我们也期望产生相对论的喷气机（或``''''），并具有相应的光束发射模式。
We first derive a set of equations describing general stationary configurations of relativistic force-free plasma, without assuming any geometric symmetries. We then demonstrate that electromagnetic interaction of merging neutron stars is necessarily dissipative due to the effect of electromagnetic draping - creation of dissipative regions near the star (in the single-magnetized case) or at the magnetospheric boundary (in the double-magnetized case). Our results indicate that even in the single magnetized case we expect that relativistic jets (or ``tongues'') are produced, with correspondingly beamed emission pattern.
