Gravitational wave physics and astronomy: Genesis(重力波物理学・天文学:創世記)
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The Second annual symposium of the innovative area
 "Gravitational Wave Physics and Astronomy: Genesis"

The Second Annual Area Symposium
Dates: 2018, Nov 26th  - Nov. 28th 
Venue: Panasonic Auditorium at YITP of Kyoto University
Dead lines: Oct. 10th(Wed): Financial supports
                      Nov. 7th(Wed): Talk and banquet registration
                      You are required to have your login-ID for registration. If you are not holding an account at this gw-genesis web site, contact us at least four business days before the deadlines above. Details are in the registration page.

Purpose: This symposium is the annual symposium of the Innovative area of Gravitational Wave Physics and Astronomy:Genesis (FY2017-21). The purpose of this symposium is to report a current status of the subgroups A01-A03, B01-B03, and C01-C02. Furthermore, invited speakers will present a current status of the topics on the constraint on the modified gravitational theory by the gravitational wave observations, the star formation in the low metallicity environment, the neutron star equation of state, X-ray follow-up observation of GW170817, radio follow-up observation of GW170817, and GW from a supernova. We also plan to present a current progress of the public researches.

Invited speakers:
  • Paolo Creminelli (ICTP)
  • Akira Ohnishi (YITP)
  • Sergey Klimenko (Univ of Florida)
  • Takanori Sakamoto (Aoyama Gakuin Univ)
Reports of research projects:
  • (A01) "Testing Gravity Theories using GWs"Takahiro Tanaka (Kyoto)
  • (A02) "New developments of gravity theory research in GW physics/astronomy" Shinji Mukohyama (Kyoto)
  • (A03) "Quest for BH binary: Formation and Evolution" Kazuyuki Omukai (Tohoku)
  • (B01) "Physics and Astrophysics with GWs from binary NS coalescences, BH-NS coalescences, pulsars and magnetars” Hideyuki Tagoshi (ICRR)
  • (B02) "Gravitational Wave Sources Probed with High Energy Observations" Nobuyuki Kawai (TITech)
  • (B03) "Identifying and observing optical/infrared counterparts of GW events" Michitoshi Yoshida (NAOJ)
  • (C01) "Investigation of Supernova Mechanism via GWs" Kei Kotake (Fukuoka)
  • (C02) "Investigation of Supernova Mechanism via Neutrino" Mark R. Vagins (IPMU)
Registration fee: None
Banquet fee: See below
Banquet place: Camphora:  University Cafeteria in front of the clock tower (map)
position
banquet fee (Nov. 27th 18:45~)
employed researcher including JSPS DC fellow
 4,500yen
student
 3,000yen
Organizers (SOC): Kunihito Ioka(YITP), Kazuyuki Omukai(Tohoku U.), Nobuyuki Kawai(Tokyo Inst. of Tec), Kenta Kiuchi(YITP), Kei Kotake(Fukuoka U.), Hideyuki Tagoshi(ICRR), Takahiro Tanaka(Kyoto U.), Mark Vagins(IPMU), Takashi Hosokawa(Kyoto U.), Shinji Mukohyama(YITP), Michitoshi Yoshida(NAOJ),
Organizers (LOC): Kunihito Ioka(YITP), Kenta Kiuchi(YITP), Shinji Mukohyama(YITP), Takahiro Tanaka(Kyoto U.), Takashi Hosokawa(Kyoto U.), Kazuya Takahashi(YITP)Ryuichi Fujita(YITP)