论文标题
白矮人的潮汐破坏：理论模型和观察前景
Tidal Disruptions of White Dwarfs: Theoretical Models and Observational Prospects
论文作者
论文摘要
白色矮人星星进入潮汐半径的黑洞，带有质量$ \ Lessim $ 10^5 $ M $ _ {\ odot} $注定要被潮汐力撕开。在恒星黑洞和超级黑洞之间的质量范围内的黑洞尚未得到最终确定，因此检测潮汐破坏白矮人将为存在中等质量黑洞的存在提供明确的证据。在这篇综述中，我们介绍了由中间质量黑洞对白矮人的潮汐破坏引起的瞬态事件的理论和观察性概述。这包括讨论最新的模拟和预测属性，观察性搜索的结果，以及摘要通过即将进行的任务检测到引力波排放的潜力。
White dwarf stars that enter the tidal radius of black holes with masses $\lesssim$ $10^5$ M$_{\odot}$ are doomed to be ripped apart by tidal forces. Black holes in this mass range between stellar black holes and supermassive black holes have not been conclusively identified so the detection of a tidal disruption of a white dwarf would provide clear evidence for the existence of intermediate-mass black holes. In this review, we present a theoretical and observational overview of the transient events that result from the tidal disruptions of white dwarfs by intermediate-mass black holes. This includes discussion of the latest simulations and predicted properties, the results of observational searches, as well as a summary of the potential for gravitational wave emission to be detected with upcoming missions.
