Name: From Quarks to Neutron Stars: Insights from kHz gravitational waves
Start: 2025-04-23T09:00:00+09:00
End: 2025-04-24T18:00:00+09:00
Location: Koshiba Hall, Hongo Campus, The University of Tokyo

From Quarks to Neutron Stars: Insights from kHz gravitational waves

from Wednesday, April 23, 2025 (9:00 AM) to Thursday, April 24, 2025 (6:00 PM)

Monday, April 21, 2025
Tuesday, April 22, 2025
Wednesday, April 23, 2025

9:30 AM Registration
Registration
9:30 AM - 9:50 AM

9:50 AM Opening Remarks (Takaaki Kajita)
Opening Remarks (Takaaki Kajita)
9:50 AM - 10:00 AM
10:00 AM QUARKS AND NUCLEAR PHYSICS
10:00 AM - 11:40 AM
Contributions

10:00 AM Lessons from hot QCD matter and neutron star unknows from the nuclear physics point of view - Kenji Fukushima

10:40 AM Equation of state of QCD(-like) theory using Lattice Monte Carlo simulations - Etsuko Itou

11:10 AM Study of asymmetric nuclear matter EoS from terrestrial nuclear experiments - Tadaaki Isobe
11:40 AM Lunch Break
Lunch Break
11:40 AM - 12:40 PM

12:40 PM Coffee Break and Poster Session
Coffee Break and Poster Session
12:40 PM - 1:10 PM
1:10 PM NEUTRON STARS AND SUPERNOVAE
1:10 PM - 3:00 PM
Contributions

1:10 PM Investigating ultra-high-density equations of state through gravitational waves from binary neutron stars mergers - Luca Baiotti

1:50 PM Diversity in neutron star merger remnants and their electromagnetic signatures - Kenta Hotokezaka

2:30 PM Testability of the quark-hadron transition using gravitational waves from merging binary neutron stars - Reiko Harada
3:00 PM Workshop Photo
Workshop Photo
3:00 PM - 3:10 PM

3:10 PM Coffee Break and Poster Session
Coffee Break and Poster Session
3:10 PM - 3:40 PM
3:40 PM NEUTRON STARS AND SUPERNOVAE
3:40 PM - 5:40 PM
Contributions

3:40 PM Gravitational-wave signatures from multi-dimensional core-collapse supernova modeling - Kei Kotake

4:20 PM Oscillation and deformation on neutron stars leading to GW detection - Yasufumi Kojima

5:00 PM Probing the Dense Matter Equation of State via Gravitational-Wave Asteroseismology - Tianqi Zhao
6:00 PM Banquet
Banquet
6:00 PM - 8:00 PM
Thursday, April 24, 2025
9:20 AM GRAVITATIONAL WAVES
9:20 AM - 10:40 AM
Contributions

9:20 AM Gravitational Wave Discoveries — Now and the Near Future - Ling Sun

10:00 AM Astrophysics and fundamental physics with NEMO -- a kHz gravitational-wave observatory - Paul Lasky
10:40 AM Coffee Break and Poster Session
Coffee Break and Poster Session
10:40 AM - 11:10 AM
11:10 AM GRAVITATIONAL WAVES
11:10 AM - 12:15 PM
Contributions

11:10 AM Possible High Frequency Upgrade of KAGRA - Yoichi Aso

11:40 AM Advanced techniques to further improve the kHz sensitivity - Kentaro Somiya
12:15 PM Lunch Break
Lunch Break
12:15 PM - 1:15 PM

1:15 PM Coffee Break and Poster Session
Coffee Break and Poster Session
1:15 PM - 1:40 PM
1:40 PM MULTIMESSENGER OBSERVATIONS
1:40 PM - 3:00 PM
Contributions

1:40 PM Optical and infrared observations of kilonovae - Masaomi Tanaka

2:20 PM Optical followup observations of multi-messenger transient events - Yuu Niino
3:00 PM Coffee Break and Poster Session
Coffee Break and Poster Session
3:00 PM - 3:30 PM
3:30 PM MULTIMESSENGER OBSERVATIONS
3:30 PM - 4:50 PM
Contributions

3:30 PM The search for X-ray counterparts of gravitational wave events - Motoko Serino

4:10 PM Multi-messenger astronomy with high energy neutrinos - Nobuhiro Shimizu
4:50 PM Closing Remarks (Tesuo Hatsuda)
Closing Remarks (Tesuo Hatsuda)
4:50 PM - 5:00 PM

Choose timezone