论文标题
部分可观测时空混沌系统的无模型预测
The Enigma of GLEAM-X~J162759.5-523504.3
论文作者
论文摘要
It is proposed that GLEAM-X~J162759.5-523504.3, the newly discovered radio transient with an unusually long spin-period (P$_s$ = 1091.1690s), can be identified to be a Radio Magnetar which has a dipolar surface magnetic field of $2.5 \times 10^{16}$~G.结果表明 - a）可以将这种强场锚定在中子星的核心 - 壳边界上，b）田间耗散的能量可以解释该来源的观察到的光度（无线电和X射线）。
It is proposed that GLEAM-X~J162759.5-523504.3, the newly discovered radio transient with an unusually long spin-period (P$_s$ = 1091.1690s), can be identified to be a Radio Magnetar which has a dipolar surface magnetic field of $2.5 \times 10^{16}$~G. It is shown that - a) it is possible to anchor such a strong field at the core-crust boundary of a neutron star, and b) the energy of field dissipation can explain the observed luminosity (radio & X-ray) of this source.
