论文标题
来自磁化白矮人的连续重力波
Continuous gravitational wave from magnetized white dwarfs
论文作者
论文摘要
从观察到过度发光的IA型超新星(Sneia)的观察结果,超级chandrasekhar白矮人(WDS)的最新证据一直是一个很好的天体物理发现。但是,到目前为止,没有直接观察到如此庞大的WD,因为它们的亮度通常很低。因此,它立即提出了一个问题,即是否有可能直接检测它们。搜索超级冠军WD非常重要,因为Sneia被用作宇宙学的标准蜡烛。在本文中,我们表明,连续重力波可以使我们能够直接检测到这种超级chandrasekhar wds。
Recent evidence of super-Chandrasekhar white dwarfs (WDs), from the observations of over-luminous type Ia supernovae (SNeIa), has been a great astrophysical discovery. However, no such massive WDs have so far been observed directly as their luminosities are generally quite low. Hence it immediately raises the question of whether there is any possibility of detecting them directly. The search for super-Chandrasekhar WDs is very important as SNeIa are used as standard candles in cosmology. In this article, we show that continuous gravitational wave can allow us to detect such super-Chandrasekhar WDs directly.