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Astrophysics of LIGO/Virgo sources in O3 era
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Lecture Hall (Kavli IPMU, Kashiwa, Japan)
Lecture Hall
Kavli IPMU, Kashiwa, Japan
Kashiwa, Japan
Description
Astrophysics of LIGO/Virgo sources in O3 era
Dates: January 20-24, 2020
Venue: Lecture Hall, Kavli IPMU, Kashiwa, Japan
Overview:
The primary goal of this workshop is the interpretation of LIGO/Virgo
detections of black hole and neutron star mergers available from
the ongoing LIGO/Virgo third observational run (O3). If results of O3
run are not yet available by January 2020, the main focus will be placed
on preparations to use the near future data to infer astrophysical
information from LIGO/Virgo detections. Our team of experts is uniquely
positioned to address and derive new astrophysical information from
LIGO/Virgo observations. We intend to discuss core-collapse and
pair-instability supernovae, NS/BH masses, angular momentum transport
in massive stars, NS/BH natal kicks, RLOF and CE phases of binary
evolution and cosmic star formation and chemical evolution. At the time
of the workshop, the Japanese KAGRA may actually be operational and
supporting LIGO/Virgo detections and we plan to invite local experts to
join us in the discussions.
Organizers :
Chris Belczynski (Polish Academy of Sciences, Poland)
Ken'ichi Nomoto (Kavli IPMU, Japan)
Naoki Yoshida (UTokyo/Kavli IPMU, Japan)
Naoki Yasuda (Kavli IPMU, Japan)
Address:
Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU),
The University of Tokyo, 5-1-5 Kashiwa-no-ha, Kashiwa City, Chiba 277-8583, Japan
Contact
The agenda of this meeting is empty
