Program
Last Update: 2016/07/28 22:49:15
All talks and slides have to be prepared in English.
Date | Morning | Afternoon 1 | Afternoon 2 |
---|---|---|---|
July 25th | |
Opening, Nova, SN | FRB |
July 26th | FRB, SNR | SNR, BBH | GRB |
July 27th | NSM | |
|
"*" symbols on talk titles mean that the presentation files are not available at the moment.
25th July (Monday)
Opening, Nova, SN (13:00-15:20)
Time | Name + Title | Institute |
---|---|---|
Chair: Toshikazu Shigeyama | ||
13:00-13:20 (15+5) | Shigehiro Nagataki | RIKEN |
Current Status & Future Prospects of ABBL & iTHES | ||
13:20-13:55 (30+5) | Kentaro Wada | U-Tokyo, RESCEU |
Nova wind acceleration through early super soft x-ray source phase and super Eddington luminosity | ||
13:55-14:20 (20+5) | Kazuhiro Noda | U-Tokyo, RESCEU |
Theoretical expectations on surviving companions in type Ia SNRs | ||
14:20-14:45 (20+5) | Malia Jenks | U-Oklahoma |
Studying Supernova physics with the Nearby Supernova factory spectro-photometric time series * | ||
14:45-15:20 (30+5) | Keiichi Maeda | Kyoto U |
Observational Constraints on Supernova Progenitor Evolution |
Coffee break (15:20-15:50)
FRB (15:50-17:35)
Time | Name + Title | Institute |
---|---|---|
Chair: Toshikazu Shigeyama | ||
15:50-16:25 (30+5) | Tomonori Totani | U-Tokyo, Astronomy |
Recent Topics about Fast Radio Bursts * | ||
16:25-17:00 (30+5) | Shotaro Yamasaki | U-Tokyo, Astronomy |
Testing double neutron star merger model for FRBs with numerical-relativity hydrodynamical simulations | ||
17:00-17:35 (30+5) | Susumu Inoue | RIKEN |
FRBs as cosmological probes |
26th July (Tuesday)
FRB, SNR (10:00-12:10)
Time | Name + Title | Institute |
---|---|---|
Chair: Shigehiro Nagataki | ||
10:00-10:35 (30+5) | Annop Wongwathanarat | RIKEN |
Neutron star kicks by gravitational tug boat mechanism | ||
10:35-11:10 (30+5) | Takashi Moriya | NAOJ |
Supernovae powered by magnetars that transform into black holes | ||
11:10-11:35 (20+5) | Miyu Masuyama | U-Tokyo, RESCEU |
Evolution of magnetar-powered supernovae | ||
11:35-12:10 (30+5) | Satoru Katsuda | Chuo U |
High-Resolution X-Ray Spectroscopy of Supernova Remnants |
Lunch (12:10-13:20)
SNR, BBH (13:20-15:05)
Time | Name + Title | Institute |
---|---|---|
Chair: Takuma Suda | ||
13:20-13:55 (30+5) | Herman (Shiu-Hang) Lee | ISAS / JAXA |
Current trends and prospects in SNR research - where we are now and where to go | ||
13:55-14:30 (30+5) | Masaomi Ono | Kyushu U |
Multi-dimensional numerical modeling of supernova remnants | ||
14:30-15:05 (30+5) | Tomoya Kinugawa | U-Tokyo, ICRR |
Binary black hole remnants of First stars for the gravitational wave source * |
Coffee break (15:05-15:35)
GRB (15:35-18:30)
Time | Name + Title | Institute |
---|---|---|
Chair: Shigehiro Nagataki | ||
15:35-16:10 (30+5) | Hirotaka Ito | RIKEN |
Physics of Relativistic Radiation Mediated Shocks | ||
16:10-16:45 (30+5) | Ayako Ishii | Tohoku U |
Study of GRB Emission Process Coupled Computation of Radiative Transfer with Relativistic Hydrodynamics | ||
16:45-17:20 (30+5) | Wataru Ishizaki | U-Tokyo, ICRR |
Spatial Profile of the Emission from Pulsar Wind Nebulae with steady-state 1D Modeling | ||
17:20-17:55 (30+5) | Haoning He | UCLA / PMO |
Monte Carlo Bayesian search for the plausible source of the Telescope Array hotspot | ||
17:55-18:30 (30+5) | Jin Matsumoto | RIKEN |
Condition for the growth of the Rayleigh-Taylor instability at the relativistic jet interface |
Banquet (19:00 @ Miyamoto Restaurant 宮本)
27th July (Wednesday)
NSM (10:00-12:20)
Time | Name + Title | Institute |
---|---|---|
Chair: Keiichi Maeda | ||
10:00-10:35 (30+5) | Don Warren | RIKEN |
Nonlinear cosmic ray acceleration in GRB afterglows | ||
10:35-11:10 (30+5) | Oliver Just | MPA |
Neutrino-driven jets and heavy element production in neutron-star mergers | ||
11:10-11:45 (30+5) | Koutarou Kyutoku | RIKEN |
The unreasonable weakness of r- process cosmic rays in the neutron- star-merger nucleosynthesis scenario | ||
11:45-12:20 (30+5) | Yutaka Komiya | U-Tokyo, RESCEU |
Contribution of neutron star merger to the r-process chemical evolution |