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Kyoto
List of Registered Participants
Tentative Program
[R] 45min + 15min
[I] 25min + 5min
[C] 12min + 3min
Monday, Oct. 29th
9:00
Registration Desk Opens
9:50-11:00
Session 1
[S]
Misao Sasaki, SOC, & LOC
Opening Address
[R]
John Wise
First Galaxies
11:00-11:20
Coffee Break
11:20-12:35
Session 2
[R]
Juntai Shen
Structures, Dynamics, and Formation of the Milky Way: A Narrow Perspective
[C]
Greg Stinson
Making Galaxies in a Cosmological Context (MaGICC)
12:35-14:00
Lunch
14:00-15:30
Session 3
[I]
Kohji Yoshikawa
Vlasov-Poisson simulations of collisionless self-gravitating systems
[C]
Qi Guo
The limits of subhalo abundance matching
[C]
Go Ogiya
Landau resonance and the core-cusp problem in cold dark matter halos
[C]
Taira Oogi
Size evolution of early-type galaxies through dry mergers
[C]
Hesti R.T. Wulandari
Impact of Orbital Eccentricity on the Capture of WIMP Dark Matter by Stars in the Galactic Center
15:30-15:50
Coffee Break
15:50-17:00
Session 4
[I]
Hyesung Kang
Particle Acceleration at Astrophysical Shocks
[C]
Franco Vazza
The injection and evolution of cosmic ray hadrons in cosmological simulations
[P]
Short Presentation of Posters part 1
17:00
Poster Viewing (with drinks and light snacks) at the ground floor in the main building
Tuesday, Oct. 30th
9:30-10:45
Session 5
[R]
Tom Abel
Following Dark Matter into Phase Space
[C]
Marcel Zemp
Molecular Hydrogen based Star Formation
10:45-11:05
Coffee Break
11:05-12:35
Session 6
[R]
Miguel-Angel Aloy
Gamma-ray burst jets
[C]
Jin Matsumoto
Effect of Interacting Rarefaction Waves on Relativistically Hot Jets
[C]
Akira Mizuta
Jet Opening angle of gamma-ray burst outflows
12:35-14:00
Lunch
14:00-15:30
Session 7
[I]
Yuichiro Sekiguchi
Merger of Binary Neutron Stars
[C]
Kenta Kiuchi
General relativistic simulation of black-hole neutron star binary mergers
[C]
Ke-Jung Chen
3D Simulations of Thermonuclear Supernovae from the Most Massive Stars
[C]
Yudai Suwa
Numerical Simulation of Core-Collapse Supernovae
[C]
Sergey Moiseenko
Implicit Lagrangian method on variable triangular grid for magnetorotational supernova simulations
15:30-15:50
Coffee Break
15:50-17:00
Session 8
[C]
Michele Montgomery
Missing Physics in Simulations of Accretion Disks
[C]
Motoyuki Saijo
Nonlinear effect of r-mode instability in uniformly rotating stars
[P]
Short Presentation of Posters part 2
17:00
Poster Viewing (with drinks and light snacks) at the ground floor in the main building
Wednesday, Oct. 31st
9:30-11:00
Session 9
[I]
Xian Chen
Tidal Stellar Disruption by Binary Supermassive Black Holes
[I]
Ken Ohsuga
Radiation Magnetohydrodynamics of Black Hole Accretion Flows and Outflows
[C]
Kinsuk Giri
Numerical simulations of a Two Component Advective Flow: Is The Flow Stable?
[C]
Tomohisa Kawashima
Hot Spine and Compton-Cooled Sheath Structure of Radiation MHD Jet: Observational Feature of Super-Eddington Black Hole Accretion Flow with Outflow
11:00-11:20
Coffee Break
11:20-12:35
Session 10
[C]
Yohei Miki
Galaxy Merger and Hungry Black Hole: Suppression of Black Hole Activity due to Galaxy Merger
[C]
Ataru Tanikawa
Merger growth of a massive black hole in a primordial galaxy: conditions for successive merger of multiple massive black holes
[C]
Takanobu Kirihara
Galaxy Collision and the Outer Density Profile in Andromeda Galaxy
[C]
Ryoji Matsumoto
Global Three-dimensional Magnetohydrodynamic Simulations of Disk Dynamos
[C]
Alexander M. Beck
Simulating Magnetic Fields in Interacting Galaxies and Forming Galactic Halos
12:35-14:00
Lunch
14:00-15:15
Session 11
[R]
Axel Brandenburg
Dynamos in astrophysics
[C]
Youhei Masada
Mean Field Generation in Local Convective Dynamo Simulation
[C]
Federico A. Stasyszyn
Global Mean Field Dynamo simulations with SPMHD
15:30-15:50
Coffee Break
15:50-17:20
Session 12
[I]
Lin-Ni Hau
Magnetic Reconnection in Space Plasmas
[C]
Hoonkyu Kim
Inverse Energy Cascade and Imbalanced Magnetohydrodynamic Turbulence
[C]
Hyunju Yoo
Effects of forcing scale on MHD turbulence
[C]
Maarten Baes
Monte Carlo dust radiative transfer with SKIRT
[C]
Yipeng Jing
A new subhalo finder: Hierarchical Bound-Tracing code
Thursday, Nov. 1st
9:30-11:00
Session 13
[R]
Ralf Klessen
(cancelled)
Star Formation Throughout the Cosmic Ages
[I]
Tomoaki Matsumoto
Protostellar collapse of magneto-turbulent cloud cores: formation of protoplanetary disks and outflows
11:00-11:20
Coffee Break
11:20-12:20
Session 14
[I]
Ruben Krasnopolsky
Theoretical Difficulties in Forming Rotationally Supported Disks
[C]
Kengo Tomida
Formation of Protostellar Cores and Circumstellar Disks
[C]
Kohji Tomisaka
Expected Observations of Star Formation Process: from Molecular Cloud Core to First Hydrostatic Core
12:20-13:40
Lunch
13:40-15:25
Session 15
[R]
Ing-Guey Jiang
Debris Disks and Planetary Systems
[C]
He-Feng Hsieh
On the secular behavior of dusts in an eccentric protoplanetary disk with an embedded massive planet
[C]
Akimasa Kataoka
Static Compression Process of Dust Aggregates in Protoplanetary Disks
[C]
Eiichiro Kokubo
The final stage of terrestrial planet formation
15:25-15:45
Coffee Break
15:45-17:00
Session 16
[C]
Hyunjin Cho
Density Distribution Functions in Supersonic Turbulence
[C]
Tsuyoshi Inoue
Formation of Turbulent and Magnetized Molecular Clouds
[C]
Elizabeth Tasker
How to kill a Giant Molecular Cloud
[C]
Ui-Han Zhang
Nonlinear instability of the cold cloud in a two-phase interstellar medium
[C]
Yuta Asahina
Magnetohydrodynamic Simulations of the Formation of Molecular Clouds in Our Galactic Center
18:30-20:30
Banquet at Kyoto Univ. Clock Tower
10 min. walk from the conference site.
All participants are invited.
Friday, Nov. 2nd
9:30-10:45
Session 17
[R]
Junichiro Makino
High Performance Computing for Cosmological Simulation
[C]
Tomoaki Ishiyama
The Gravitational Trillion-Body Problem on K computer
10:45-11:05
Coffee Break
11:05-12:20
Session 18
[R]
Jae-Min Kwon
Gyro-kinetic Simulation: Introduction and Prospect for Astrophysics
[C]
Yosuke Matsumoto
Electron accelerations at high Mach number shocks: Two-dimensional Particle-in-Cell simulations on massively parallel supercomputer systems
12:20-14:00
Lunch
14:00-15:30
Session 19
[I]
Dongwook Lee
FLASH for Astrophysics, High-Energy-Density Physics, and more...
[C]
Tomoyuki Hanawa
Reconstruction Method for Solving M1 Equations for Radiative Transfer
[C]
Hanbyul Jang
A Relativistic Magnetohydrodynamic Code Based on an Upwind Scheme
[C]
Tsungche Liu
Web-based Cloud Computing for High Energy Neutrino Simulation
[C]
Hung-Hsu Chan
A New Method for Computation of Self-Gravity in an Isolated System
15:30-16:00
Session 20
[S]
Summary