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2016 Fiscal Year Final Research Report

New development in astrophysics through multi messenger observation of gravitational wave sources

Organizer

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Project AreaNew development in astrophysics through multimessenger observations of gravitational wave sources
Project/Area Number 24103001
Research Category

Grant-in-Aid for Scientific Research on Innovative Areas (Research in a proposed research area)

Allocation TypeSingle-year Grants
Review Section Science and Engineering
Research InstitutionKyoto University

Principal Investigator

Nakamura Takashi  京都大学, 理学研究科, 名誉教授 (80155837)

Co-Investigator(Kenkyū-buntansha) 田中 貴浩  京都大学, 理学(系)研究科(研究院), 教授 (40281117)
神田 展行  大阪市立大学, 理学(系)研究科(研究院), 教授 (50251484)
河合 誠之  東京工業大学, 理工学研究科, 教授 (80195031)
吉田 道利  広島大学, 学内共同利用施設等, 教授 (90270446)
ヴァギンズ マーク  東京大学, 学内共同利用施設等, 教授 (90509902)
Co-Investigator(Renkei-kenkyūsha) KAJITA Takaaki  東京大学, 宇宙線研究所, 教授 (40185773)
SASAKI Misao  京都大学, 基礎物理学研究所, 教授 (70162386)
TSUBONO Kimio  東京大学, 理学研究科, 教授 (10125271)
ITOH Yoshitaka  名古屋大学, 太陽地球環境研究所, 教授 (50272521)
WATANABE Jyunichi  国立天文台, 教授 (50201190)
Project Period (FY) 2012-06-28 – 2017-03-31
Keywords重力波 / X線・ガンマ線観測 / 光学赤外観測 / ニュートリノ観測 / データ解析 / 重力波の理論
Outline of Final Research Achievements

Sep. 14 in 2015, the first direct detection of gravitational waves was done by the detectors in USA. The source of the gravitational waves was the merger of the massive black hole binary of mass about 30 solar mass. This was unexpected source for many researchers in this field. However this innovative area predicted in 2014 the existence of such black hole binary formed from the zero metal first stars in the Universe and the possible detections in 2015. In the paper announced this discovery, our prediction was written as the astonishing agreement between the observed mass and the predicted one. Similar source was observed Jan. 4th in 2017 so that our prediction would be confirmed in future. This innovative area performed the follow-up observations by X-ray, optical radiation, neutrino and data analysis simultaneously with the gravitational wave observations.

Free Research Field

宇宙物理学

URL: 

Published: 2018-03-22  

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