论文标题
中子星二进制系统的多理解剂可观察性
Multi-Messenger Observability of Neutron Star Binary System
论文作者
论文摘要
随着技术的改进，二进制中性星系的观察到更频繁的频率，实际上，具有电磁对应物的第一个引力波源自两个中子星的合并（GW170817）。在合并之前检测这些系统可能有助于恢复基本数据，以开发中子恒星的状态方程。本文通过模拟光学中的中子恒星系统的潜在可观察性，研究了在合并之前脱落的二进制中子星的可观察性。发现由于可见性较低和时间分辨率不足，因此不太可能考虑当前的仪器，但是，将来的改进或宽场X射线仪器可能会为检测这些系统提供可行的选择。
As technology has improved, binary neutron star systems have been observed more frequently, in fact, the first gravitational wave to have an electromagnetic counterpart originated from the merger of two neutron stars (GW170817). Detecting these systems prior to merger may help recover essential data for developing an Equation of State for neutron stars. This paper examines the observability of detached eclipsing binary neutron stars prior to merger by simulating the potential observability of neutron star systems in the optical. It is found that it is not likely considering current instruments due to low visibility and inadequate time resolution, however, improvements in the future or a wide field X-ray instrument may offer a viable option for detecting these systems.
