Program
Last Update: 2019/03/22 14:58:23
All talks and slides are recommended to be prepared in English.
| Date | Morning | Afternoon 1 | Afternoon 2 |
|---|---|---|---|
| March 19th | Opening, SN | GRB | SN |
| March 20th | SN, SNR | NSM | SN |
19th March (Tuesday)
Opening, SN (11:00-12:30)
| Time | Name + Title | Institute |
|---|---|---|
| Chair: Ayako Ishii | ||
| 11:00-11:20 (15+5) | Toshikazu Shigeyama | U-Tokyo, RESCEU |
| Opening, A bright supernova SN 2012au hosting a pulsar |
||
| 11:20-12:00 (35+5) | Takashi J. Moriya | NAOJ |
| Circumstellar properties of Type Ia supernovae with helium star donors | ||
| 12:00-12:30 (25+5) | Kazumi Kashiyama | U-Tokyo, RESCEU |
| X-raying the Birth of Binary Neutron Stars | ||
Lunch break (12:30-14:00)
GRB (14:00-15:40)
| Time | Name + Title | Institute |
|---|---|---|
| Chair: Toshikazu Shigeyama | ||
| 14:00-14:40 (35+5) | Hirotaka Ito | ABBL, RIKEN |
| Relativistic Radiation Mediated Shocks | ||
| 14:40-15:10 (25+5) | Don Warren | iTHEMS, RIKEN |
| Thermal electrons in GRB afterglows: causes and effects | ||
| 15:10-15:40 (25+5) | Akira Mizuta | RIKEN |
| 3D GRMHD simulation of black hole accretion flows and jets | ||
Coffee break (15:40-16:10)
SN (16:10-17:40)
| Time | Name + Title | Institute |
|---|---|---|
| Chair: Kazumi Kashiyama | ||
| 16:10-16:50 (35+5) | Akira Harada | U-Tokyo, UTAP |
| Core-collapse Supernova Simulations with the Boltzmann-neutrino-transport | ||
| 16:50-17:15 (20+5) | Yuki Takei | U-Tokyo, RESCEU |
| Constructing a Model for Interaction-Powered Supernovae | ||
| 17:15-17:40 (20+5) | Daichi Tsuna | U-Tokyo, RESCEU |
| A Light Curve Model of Interaction-Powered Supernovae | ||
Banquet 18:30กม
20th March (Wednesday)
SN, SNR (10:00-12:35)
| Time | Name + Title | Institute |
|---|---|---|
| Chair: Takashi Moriya | ||
| 10:00-10:40 (35+5) | Gilles Ferrand | ABBL, RIKEN |
| From the (thermonuclear) supernova to the supernova remnant | ||
| 10:40-11:10 (25+5) | Masaomi Ono | RIKEN |
| Three dimensional simulation from supernova explosions to their supernova remnants: the dynamical and chemical evolution of SN 1987A | ||
| 11:10-11:40 (25+5) | Takuma Suda | U-Tokyo, RESCEU |
| Core-collapses supernova explosions in binary systems as a probe into Pop. III stars | ||
| 11:40-12:10 (25+5) | Kotaro Fujisawa | Waseda University |
| Effects of rotation and magnetic field on the revival of a stalled shock in supernova explosions | ||
| 12:10-12:35 (20+5) | Kenichi Sugiura | Waseda University |
| Linear Analysis of the Shock Instability in Core-collapse Supernovae | ||
Lunch break (12:35-14:00)
NSM (14:00-15:55)
| Time | Name + Title | Institute |
|---|---|---|
| Chair: Takuma Suda | ||
| 14:00-14:40 (35+5) | Tomoya Kinugawa | U-Tokyo |
| Metallicitydependence of BH+MS binaries detectable with Gaia, Rate ofultra-stripped supernovae and binary evolution leading to double NS |
||
| 14:40-15:10 (25+5) | Oliver Just | ABBL, RIKEN |
| Outflows From Neutron-Star Mergers | ||
| 15:10-15:40 (25+5) | Haoxiang Lin | U-Tokyo |
| GW170817 afterglow: a more natural electron energy distribution leads to a new solution | ||
| 15:40-15:55 (12+3) | Yongjia Huang | iTHEMS, RIKEN |
| Introduction to simulate BNS mergers via Einsteintoolkit | ||
Coffee break (15:55-16:20)
SN (16:20-18:25)
| Time | Name + Title | Institute |
|---|---|---|
| Chair: Kotaro Fujisawa | ||
| 16:20-17:00 (35+5) | Chinami Kato | Waseda University |
| Effects of nucleon recoils for neutrino spectra in core-collapse supernovae | ||
| 17:00-17:30 (25+5) | Haoning He | ABBL, RIKEN |
| On the Origin of IceCube High Energy Neutrinos | ||
| 17:30-18:00 (25+5) | Milad Delfan Azari | Waseda University |
| Linear analysis of fast pair-wise collective neutrino oscillations in CCSNe based on the results of realistic Boltzmann simulations | ||
| 18:00-18:25 (20+5) | Masamichi Zaizen | U-Tokyo |
| Collective neutrino oscillations and matter effects in core-collapse supernovae | ||