Prospects for Detection of Extragalactic Stellar Black Hole Binaries in the Nearby Universe

被引:0
|
作者
Benacquista, Matthew [1 ]
Hinojosa, Jesus [1 ]
Mata, Alberto [1 ]
Belczynski, Krzysztof [1 ,2 ]
机构
[1] Univ Texas Brownsville, Ctr Gravitat Wave Astron, Brownsville, TX 78520 USA
[2] Univ Warsaw, Astron Observ, PL-00478 Warsaw, Poland
来源
10TH INTERNATIONAL LISA SYMPOSIUM | 2015年 / 610卷
关键词
D O I
10.1088/1742-6596/610/1/012049
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Stellar mass black hole binaries have individual masses between 10-80 solar masses. These systems may emit gravitational waves at frequencies detectable at Megaparsec distances by space-based gravitational wave observatories. In a previous study, we determined the selection effects of observing these systems with detectors similar to the Laser Interferometer Space Antenna by using a generated population of binary black holes that covered a reasonable parameter space and calculating their signal-to-noise ratio. We further our study by populating the galaxies in our nearby (less than 30 Mpc) universe with binary black hole systems drawn from a distribution found in the Synthetic Universe to ultimately investigate the likely event rate of detectable binaries from galaxies in the nearby universe.
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页数:4
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