The Bulletin of The Korean Astronomical Society (천문학회보)
- Volume 42 Issue 2
- /
- Pages.53.3-53.3
- /
- 2017
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- 1226-2692(pISSN)
Binary Black Hole Inspirals and GW detection in 0.1-10 Hz
- Bae, Yeong-Bok (Korea Astronomy & Space Science Institute) ;
- Ahn, Sang-Hyeon (Korea Astronomy & Space Science Institute) ;
-
Kang, Gungwon
(Korea Institute of Science and Technology Information)
;
- Kim, Chunglee (Korea Astronomy & Space Science Institute) ;
- Kim, Whansun (National Institute for Mathematical Sciences) ;
- Oh, John J. (National Institute for Mathematical Sciences) ;
-
Oh, Sang Hoon
(National Institute for Mathematical Sciences)
;
- Park, Chan (Korea Institute of Science and Technology Information) ;
- Son, Edwin J. (National Institute for Mathematical Sciences) ;
- Lee, Yong Ho (Korea Research Institute of Standards and Science)
- Published : 2017.10.10
Abstract
The pilot study of SLGT (Superconducting Low-frequency Gravitational-wave Telescope) is being performed by KKN (KASI-KISTI-NIMS) collaboration. In this presentation, we discuss prospectives of detecting GWs in the low-frequency band (0.1-10 Hz), which is a target frequency band of SLGT, but can be hardly observed by advanced LIGO. IMBHBs (Intermediate Mass Black Hole Binaries) and IMRIs (Intermediate Mass Ratio Inspirals) with total masses of O(1000) up to O(10,000) solar masses are most probable sources between 0.1-10 Hz. We estimate horizon distances and signal to noise ratios of IMBHBs and IMRIs for different SLGT design sensitivities. Based on our calculations, detection rates for IMBHBs and IMRIs with SLGT will be discussed.
Keywords