论文标题
用于检测超级chandrasekhar白色矮人的时间尺度
Timescales for detection of super-Chandrasekhar white dwarfs by gravitational wave astronomy
论文作者
论文摘要
在过去的几十年中，从间接观察中违反白矮人的chandrasekhar质量限制的推论可能是天文学中的革命性发现。各种研究人员已经提出了不同的理论来解释这一有趣的现象。但是，这种庞大的白色矮人通常具有很少的光度，因此，到目前为止，无法直接检测到任何观察结果。我们已经提出，连续重力波可能是直接检测它们的探针之一，将来，诸如Lisa，Decigo和BBO等各种基于空间的探测器应该能够检测到许多白矮人（前提是它们的表现都像脉搏）。在本文中，我们解决了与重力和偶极辐射的发射有关的各个时间尺度。这种探索为探测器设定了一个时间范围，以观察大量的白色矮人。
In about last couple of decades, the inference of the violation of the Chandrasekhar mass-limit of white dwarfs from indirect observation is probably a revolutionary discovery in astronomy. Various researchers have already proposed different theories to explain this interesting phenomenon. However, such massive white dwarfs usually possess very little luminosity, and hence they, so far, cannot be detected directly by any observations. We have already proposed that the continuous gravitational wave may be one of the probes to detect them directly, and in the future, various space-based detectors such as LISA, DECIGO, and BBO, should be able to detect many of those white dwarfs (provided they behave like pulsars). In this paper, we address various timescales related to the emission of gravitational as well as dipole radiations. This exploration sets a timescale for the detectors to observe the massive white dwarfs.
