Low-Latency Compact Object Searches with LIGO, Virgo and KAGRA in O2 and O3
| Project/Area Number |
16H06714
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| Research Category |
Grant-in-Aid for Research Activity Start-up
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| Allocation Type | Single-year Grants |
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| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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| Research Institution | The University of Tokyo |
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Principal Investigator |
Cannon Kipp 東京大学, 大学院理学系研究科(理学部), 准教授 (50777886)
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| Project Period (FY) |
2016-08-26 – 2018-03-31
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| Project Status |
Completed (Fiscal Year 2018)
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| Budget Amount *help |
¥2,990,000 (Direct Cost: ¥2,300,000、Indirect Cost: ¥690,000)
Fiscal Year 2017: ¥1,430,000 (Direct Cost: ¥1,100,000、Indirect Cost: ¥330,000)
Fiscal Year 2016: ¥1,560,000 (Direct Cost: ¥1,200,000、Indirect Cost: ¥360,000)
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| Keywords | gravitational wave / black hole / neutron star / LIGO / Virgo / KAGRA / signal processing / gravitational waves / astrophysics / 宇宙物理 / black holes / neutron stars / experimental gravity |
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| Outline of Final Research Achievements |
This project had two main goals: (i) generalize the GstLAL gravitational-wave signal detection system (https://wiki.ligo.org/Computing/DASWG/GstLAL) so that it will be able to process data from the future Japanese KAGRA detector; (ii) search for gravitational waves from black hole and neutron star collisions in Advanced LIGO and Advanced Virgo's second observing run. Both goals were achieved. Notable among the accomplishments was the GstLAL detection system's discovery of GW170817, the first gravitational wave from a neutron star collision.
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| Academic Significance and Societal Importance of the Research Achievements |
The discovery of GW170817 altered our understanding of the origin of heavy elements, and showed us that gravity moves at the speed of light, which had a significant impact on our understanding of the nature of gravity.
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Report
(3 results)
Research Products
(9 results)
