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引用次数: 1
摘要
在黑洞-中子星双星的后期吸气中磁场的存在可能导致潜在的可探测的电磁前体瞬变。利用广义相对论的无力电动力学模拟,我们研究了黑洞-中子星系统共同磁层的合并前相互作用。我们证明了这些系统可以具有丰富的电磁耀斑活动,我们发现这取决于磁场方向,而不是黑洞自旋。由于与周围磁层的相互作用,这些耀斑可能导致类似快速射电暴的瞬态和x射线发射,亮度的上限为EM > 10 41 B * / 10 12 G 2 erg s−1,其中B *是中子星表面的磁场强度。
Electromagnetic Precursors to Black Hole–Neutron Star Gravitational Wave Events: Flares and Reconnection-powered Fast Radio Transients from the Late Inspiral
Abstract The presence of magnetic fields in the late inspiral of black hole–neutron star binaries could lead to potentially detectable electromagnetic precursor transients. Using general-relativistic force-free electrodynamics simulations, we investigate premerger interactions of the common magnetosphere of black hole–neutron star systems. We demonstrate that these systems can feature copious electromagnetic flaring activity, which we find depends on the magnetic field orientation but not on black hole spin. Due to interactions with the surrounding magnetosphere, these flares could lead to fast-radio-burst-like transients and X-ray emission, with EM≲1041B*/1012G2ergs−1 as an upper bound on the luminosity, where B * is the magnetic field strength on the surface of the neutron star.
期刊介绍:
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