论文标题
连续重力波搜索的状态和观点
Status and perspectives of Continuous Gravitational Wave searches
论文作者
论文摘要
引力波天文学的诞生是通过合并两个紧凑型物体（也称为紧凑的二元聚结）所产生的信号引发的。基于地球的高级干涉仪网络对许多科学领域产生了重大影响：天体物理学，宇宙学，核物理学和基本物理学。但是，紧凑的二元聚结信号并不是Ligo，处女座和Kagra可能检测到的引力波的唯一类型。一个有趣的信号家族，以及在本综述中考虑的信号，是所谓的连续波，在典型的范式上被银河辐射由银河辐射发出的重力辐射，快速旋转的孤立的中子星在其质量分布中具有一定程度的不对称性。在这项工作中，我将回顾一下高级检测器数据分析的状态和最新结果，包括搜索暗物质签名。
The birth of gravitational wave astronomy was triggered by the first detection of a signal produced by the merger of two compact objects (also known as a compact binary coalescence event). The following detections made by the Earth-based network of advanced interferometers had a significant impact in many fields of science: astrophysics, cosmology, nuclear physics and fundamental physics. However, compact binary coalescence signals are not the only type of gravitational waves potentially detectable by LIGO, Virgo, and KAGRA. An interesting family of still undetected signals, and the ones that are considered in this review, are the so-called continuous waves, paradigmatically exemplified by the gravitational radiation emitted by galactic, fast-spinning isolated neutron stars with a certain degree of asymmetry in their mass distribution. In this work, I will review the status and the latest results from the analyses of advanced detector data, including searches for dark matter signatures.
