Strong gravitational lensing of gravitational waves in Einstein Telescope

被引:49
|
作者
Piorkowska, Aleksandra [1 ]
Biesiada, Marek [1 ]
Zhu, Zong-Hong [2 ]
机构
[1] Univ Silesia, Dept Astrophys & Cosmol, Inst Phys, PL-40007 Katowice, Poland
[2] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
关键词
gravitational lensing; gravitational waves / sources; gravitational waves / experiments; COSMIC EQUATION; GALAXIES; RATES; STATE; DARK;
D O I
10.1088/1475-7516/2013/10/022
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Gravitational wave experiments have entered a new stage which gets us closer to the opening a new observational window on the Universe. In particular, the Einstein Telescope (ET) is designed to have a fantastic sensitivity that will provide with tens or hundreds of thousand NS-NS inspiral events per year up to the redshift z = 2. Some of such events should be gravitationally lensed by intervening galaxies. We explore the prospects of observing gravitationally lensed inspiral NS-NS events in the Einstein telescope. Being conservative we consider the lens population of elliptical galaxies. It turns out that depending on the local insipral rate ET should detect from one per decade detection in the pessimistic case to a tens of detections per year for the most optimistic case. The detection of gravitationally lensed source in gravitational wave detectors would be an invaluable source of information concerning cosmography, complementary to standard ones (like supernovae or BAO) independent of the local cosmic distance ladder calibrations.
引用
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页数:12
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