Program
| Tuesday October 23, 2018 | |
|---|---|
| Session 3: Neutron-Star Merger, Relativity, Gravitational Wave Chair: Kuo-Chuan Pan (NTHU) | |
| 08:20~08:50 | Invited Binary neutron stars: Einstein's richest laboratory Luciano Rezzolla (Goethe University Frankfurt am Main, Germany) |
| 08:50~09:10 | Properties of the dynamical ejecta in binary neutron star merger and r-process nucleosynthesis Yuichiro Sekiguchi (Toho University) |
| 09:10~09:40 | Invited r-process nucleosynthesis and kilonovae Meng-Ru Wu (Institute of Physics, Academia Sinica) |
| 09:40~10:00 | Relativistic simulations of binary neutron star mergers CHIA-HUI Lin (ASIAA/NTU) |
| 10:00~10:30 | Coffee Break |
| 10:30~11:00 | Invited Numerical relativity simulations of binary-neutron-star mergers and GW170817 Koutarou Kyutoku (High Energy Accelerator Research Organization (KEK)) |
| 11:00~11:20 | Numerical-Relativity simulations of stellar collapse in Massive Scalar-Tensor gravity Patrick C. K. Cheong (The Chinese University of Hong Kong) |
| 11:20~11:40 | Hydrodynamic Simulation of Dark Matter Admixed Accretion-Induced Collapse: Gravitational-wave Signals Shuai Zha (the Chinese University of Hong Kong) |
| 11:40~12:00 | Development of GW studies in UNIST Chun-Che (Lupin) Lin (UNIST) |
| 12:00~13:20 | Lunch |
| Session 4: Interstellar Medium , Plasma, Turbulence, Shocks Chair: Min-Kai Lin (ASIAA) | |
| 13:20~13:40 | Physical properties of the multiphase interstellar medium in converging HI flow Masato Kobayashi (Osaka University) |
| 13:40~14:00 | Mathematical modeling of the formation of dense clumps in the collisions of molecular clouds Boris Rybakin (SRISA RAS, Moscow State University M.V.Lomonosov) |
| 14:00~14:20 | Anisotropic Structure of Synchrotron Polarization Hyeseung Lee (Korea Astronomy and Space Science Institute (KASI)) |
| 14:20~14:40 | Electrostatic and electromagnetic streaming instabilities in the electron-positron plasma Chun-Sung Jao (Deutsches Elektronen-Synchrotron (DESY)) |
| 14:40~15:00 | Tracing 3D B-field directions and strengths through the Velocity Gradient Technique: Review and prospect KA HO YUEN (University of Wisconsin-Madison) |
| 15:00~15:30 | Coffee Break |
| 15:30~16:00 | Invited Particle acceleration at shocks in galaxy clusters and large-scale structure Hyesung Kang (Pusan National University) |
| 16:00~16:20 | Turbulence and Magnetic fields in Galaxy Clusters: a Simulation Study Soonyoung Roh (UNIST) |
| 16:20~16:40 | Merger Shocks in Simulated Galaxy Clusters Ji-Hoon Ha (Ulsan National Institute of Science and Technology (UNIST)) |
| 16:40~17:00 | Shock Waves and their Roles in Astrophysical Turbulence Dongsu Ryu (UNIST) |
| 17:00~18:00 | Poster Reviewing (in the Discussion Room) |
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