Multimessenger astronomy with the Einstein Telescope
Multimessenger astronomy with the Einstein Telescope
复制标题
DOI：
10.1007/s10714-010-1019-z
复制
发表时间：
2010-04
影响因子：
2.8
通讯作者：
É. Chassande-Mottin;M. Hendry;P. Sutton;S. Márka
中科院分区：
文献类型：
--
作者：
É. Chassande-Mottin;M. Hendry;P. Sutton;S. Márka
引力波在多信使天体物理学的发展中起着至关重要的作用。GW观测与其他天体物理触发器的结合，例如来自伽马射线和X射线卫星，光学/射电望远镜和中微子探测器，使我们能够破译否则无法获得的科学。在本文中，我们提供了一个广泛的审查，从多信使的角度来看，提供的第三代干涉GW探测器，特别是爱因斯坦望远镜（ET）的科学范围。我们专注于宇宙瞬变，并根据我们的估计ET的前辈GEO，LIGO和处女座获得的结果。
Gravitational waves (GWs) are expected to play a crucial role in the development of multimessenger astrophysics. The combination of GW observations with other astrophysical triggers, such as from gamma-ray and X-ray satellites, optical/radio telescopes, and neutrino detectors allows us to decipher science that would otherwise be inaccessible. In this paper, we provide a broad review from the multimessenger perspective of the science reach offered by the third generation interferometric GW detectors and by the Einstein Telescope (ET) in particular. We focus on cosmic transients, and base our estimates on the results obtained by ET’s predecessors GEO, LIGO, and Virgo.