The aim of the workshop is to dicuss the signals of gravitational waves and neutrinos from core-collapse supernovae to probe into the stellar collapse and explosion as well as the birth of compact objects. The observational facilities such as Super-Kamiokande and KAGRA are prepared to detect the burst signals from the next supernova and the Super-Kamiokande with Gd loading will detect the first event of the diffuse supernova neutrino background. The cutting-edge numerical simulations are revealing the explosion mechanism with prediction of signals and exploring variety of explosive phenomena . We would like to exchange the latest understanding of observations and theories and to discuss how to extract the information from stellar core.
Topics to discuss
Program
The talks are basically arranged with the invited speakers.
Invited speakers include:
Organizers
This workshop is organized by scientific research on innovative areas 'Gravitational wave physics and astronomy : Genesis', C01 and C02 group. (Virtually Local organizer: K. Sumiyoshi, A. Harada, H. Matsufuru, Y. Koshio and M. Vagins)
Support
This work is supported by Grant-in-Aid for Scientific Research on Innovative areas "Gravitational wave physics and astronomy:Genesis" (17H06357, 17H06365)
and
Grant-in-Aid for Scientific Research (19K03837, 20H01905)
from the Ministry of Education, Culture, Sports, Science and Technology (MEXT), Japan
This workshop follows the line of the following workshops:
Deciphering multi-Dimensional nature of core-collapse SuperNovae via Gravitational-Wave and neutrino signatures (SNeGWv2018)
and
Numazu Workshop 2015: Challenges of modeling supernovae with nuclear data