EANAM7 (Beijing, China)
The Eighth East Asian Numerical Astrophysics Meeting (EANAM 2018)
October 22-26, 2018
National Cheng-Kung University (NCKU), Tainan, Taiwan

Participants

Total number: 126
1 Parisi Alessandro Tamkang University
2 waheed ali Amur 8 SHAH ABDUL LATIF UNIVERSITY KHAIRPUR
[Oral Presentation] effect of astronomy on signals and networking system
3 Shohei Aoyama Academia Sinica Institute of Astronomy and Astrophysics (ASIAA)
[Oral Presentation] Comparison of cosmological simulations and deep submillimetre galaxy surveys
4 Xuening Bai 白雪宁 Tsinghua University
5 Defu Bu Shanghai Astronomical Observatory (SHAO)
6 Zhoujian Cao Academy of Mathematics and Systems Science, Chinese Academy of Sciences
[Oral Presentation] Application of local discontinuous Galerkin method to Einstein equations
7 James Chan 詹弘旭 EPFL
[Oral Presentation] How do stars affect ψDM haloes?
8 Tzu-Hsiang Chao 趙子翔 National Taiwan University/ASIAA
[Poster] Cosmological Impact of the First Stars
9 Yeo-Yie Charng SooChow University
10 Chiang-Mei Chen 陳江梅 National Central University
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11 Chuan-Hung Chen 陳泉宏 NCKU
12 Hsin Chen NTNU
13 Ke-Jung (Ken) Chen 陳科榮 ASIAA
[Oral Presentation] How the First Supernovae Regulated Star Formation in the First Galaxies
14 Li-Hsin Chen 陳立馨 ASIAA/NTU
[Oral Presentation] Formation of the First Galaxies
15 Meng-You Chen 陳孟佑 National Cheng-kung University
16 Chia-Hsuan Cheng National Tsing Hua University
[Poster] Is There an Intermediate-Mass Black Hole in the Globular Cluster Omega Centauri ?
17 Han Cheng 鄭翰 NCU
18 Patrick C. K. Cheong 張志杰 The Chinese University of Hong Kong
[Oral Presentation] Numerical-Relativity simulations of stellar collapse in Massive Scalar-Tensor gravity
19 Pattana Chintarungruangchai 周厚發 National Tsing Hua University
[Poster] A New 2D-CNN Deep Learning Model to Search for Exoplanet Transits
20 Hing-Tong Cho 曹慶堂 Physics Department, Tamkang University
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21 Jungyeon Cho 趙, 政衍 Chungnam National University
[Oral Presentation] A modified Davis-Chandrasekhar-Fermi method
22 Wan-Hsien Cho 卓宛嫺 NCU
23 Chung-Hsien Chou 周忠憲 NCKU
24 Tzuu-Kang Chyi 齊祖康 SCU
25 Emanuele Contini 斑马 Yonsei Univeristy
[Oral Presentation] On the formation and physical properties of the intracluster light in hierarchical galaxy formation models
26 Michiko Fujii The University of Tokyo
[Oral Presentation] Modeling the Milky Way Galaxy as an N-body System
27 Yuri Fujii 藤井悠里 Nagoya University
[Oral Presentation] Radiation Hydrodynamic Simulations of the gas flow into the vicinity of gas giants
28 Liang Gao 高亮 National Astronomical Observatories, CAS
29 Hidenori Genda Earth-Life Science Institute, Tokyo Institute of Technology
[Oral Presentation] Collisions during planet and satellite formation
30 Yang Guo 郭洋 Nanjing University
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31 YanSong Guo 郭岩松 NAGOYA UNIVERSITY
[Oral Presentation] Magneto-Hydrodynamical Analysis of High-Velocity Compact Molecular Clouds
32 Ji-Hoon Ha 河知勳 Ulsan National Institute of Science and Technology (UNIST)
[Oral Presentation] Merger Shocks in Simulated Galaxy Clusters
33 Wenbiao Han 韩文标 Shanghai Astronomical Observatory
34 Tomoyuki Hanawa 花輪知幸 Chiba University
[Oral Presentation] A Numerical Scheme Ensuring Total Energy Conservation Including Self-Gravity
35 Taku Hasegawa Tokyo University
[Oral Presentation] Destruction of the Circumstellar Disk during the early period of the Cluster
36 Hiroyuki Hirashita 平下博之 ASIAA
[Oral Presentation] Evolution of dust grain size distribution in galaxies
37 Chi-Ting Ho 何基廷 Physics Department ,National Tsing Hua University
[Poster] Searching for Young Stellar Objects with Convolutional Neural Network
38 Yu-Heng Ho 賀聿恆 National Tsing Hua University
[Oral Presentation] The Effect of Impact Parameter on the Formation of Supermassive Binary Black Holes in Galactic Mergers
39 He-Feng Hsieh 謝和峯 National Tsing Hua University
[Poster] The effect of gas drag on planetesimals near mean-motion resonance
40 Yue Hu 胡越 University of Wisconsin-Madison
Top
41 Yun-Jing Huang National Taiwan University
42 Hiroki Ichihashi 市橋洋基 Hokkaido University
[Oral Presentation] Solving the cooling flow problem by introducing non gravitational dark
matter-baryon interaction
43 Taichi Igarashi Chiba Univ.
[Oral Presentation] Global Three-dimensional Radiation MagnetoHydroDynamic Simulations of Hard-to-Soft Transitions in Stellar Mass Black Hole Candidates.
44 SHUICHIRO Inutsuka Nagoya University
[Oral Presentation] An Origin of Multiple Rings in Protoplanetary Disks: Non-Linear Development of Secular Gravitational Instability in Protoplanetary Disks
45 Tomoaki Ishiyama Chiba University
[Oral Presentation] Hierarchical formation of dark matter halos near the free streaming scale and implications for annihilation signals
46 Chun-Sung Jao 饒駿頌 Deutsches Elektronen-Synchrotron (DESY)
[Oral Presentation] Electrostatic and electromagnetic streaming instabilities in the electron-positron plasma
47 Li-Wei Ji Beijing Normal University
[Oral Presentation] Solving Einstein's equations with DG method
48 Ing-Guey Jiang 江瑛貴 National Tsing Hua University
[Oral Presentation] Searching for Exoplanet Transits through a Machine Learning Technique with Convolutional Neural Network
49 Kim Jinho Korea Astronomy and Space Science Institute
[Oral Presentation] Stability of Astrophysical Jets
50 Hyesung Kang Pusan National University
[Oral Presentation] Particle acceleration at shocks in galaxy clusters and large-scale structure
Top
51 Hyosun Kim KASI
[Oral Presentation] Spiral-shell patterns surrounding evolved stars, proving binary properties
52 Yonghwi Kim 金龍輝 Korea Institute for Advanced Study
[Oral Presentation] Physical Properties of Spiral Structures: An Approach Based on the Density-Wave Theory
53 Taysun Kimm Yonsei University
[Oral Presentation] Impact of Lyman alpha pressure on metal-poor dwarf galaxies
54 Kazuki Kinjo Chiba University
[Poster] Analysis of statistical properties of dark matter subhalos using principal component analysis
55 Takanobu Kirihara Chiba University
[Oral Presentation] The nature of the progenitor of the M31 north-western stream: globular clusters as milestones of its orbit
56 Masato Kobayashi Osaka University
[Oral Presentation] Physical properties of the multiphase interstellar medium in converging HI flow
57 Tetsushi Kodama Chiba University
[Oral Presentation] Acceleration of the tree method with SIMD instruction set
58 Ilia Kondratev Space Reseach Institute; National Research nuclear University MEPhI, Moscow, Russia
[Oral Presentation] 3D operator numerical method. Application to neutron stars anisotropic heat transfer simulations.
59 Kenji Kurosaki 黒﨑健二 Nagoya University
[Oral Presentation] The Exchange of Mass and Angular Momentum in the Impact Event of Ice Giant Planets: Implications for the origin of Uranus
60 Koh Kuwabara 桑原滉 The University of Tokyo
[Oral Presentation] Growth of solid particles in protoplanetary disks with magnetically driven disk winds
Top
61 Koutarou Kyutoku 久徳浩太郎 High Energy Accelerator Research Organization (KEK)
[Oral Presentation] Numerical relativity simulations of binary-neutron-star mergers and GW170817
62 I-Hsuan Lai 賴怡璇 NTNUDepartment of Earth Sciences, NTNU
63 Hyeseung Lee Korea Astronomy and Space Science Institute (KASI)
[Oral Presentation] Anisotropic Structure of Synchrotron Polarization
64 Charles Lin Department of Earth Science, National Cheng Kung University
[Poster] Simulation of Ionospheric Instability Triggered by Typhoons
65 CHIA-HUI Lin 林家暉 ASIAA/NTU
[Oral Presentation] Relativistic simulations of binary neutron star mergers
66 Chun-Che (Lupin) Lin 林峻哲 UNIST
[Oral Presentation] Developmemt of GW studies in UNIST
67 Chun-Yu Lin 林俊鈺 National Center for High-performance Computing
68 Feng-Li Lin National Taiwan Normal University
69 Jerry Lin 林宏修 TSING HUA Unuversity
70 Min-Kai Lin 林明楷 ASIAA
[Oral Presentation] Lifting dust particles by hydrodynamic turbulence in protoplanetary disks
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71 Chun-Fan Liu 劉君帆 ASIAA
72 Chin Shan Lue National Cheng Kung University
73 Yuji Matsumoto Academia Sinica Institute of Astronomy and Astrophysics
[Poster] The formation of close-in super-Earths through in-situ giant impacts around M-dwarfs
74 Shun-Pei Miao 苗舜培 National Cheng Kung University
75 Philipp Moesta University of California at Berkeley
[Oral Presentation] Jet-driven core-collapse supernovae in the multimessenger era
76 Sergey Moiseenko Space Research Institute, Moscow, Russia
[Oral Presentation] Conservative grid functions remapping method for Lagrangian operator-difference scheme for astrophysical MHD problems.
77 Yu Morinaga Chiba University
[Oral Presentation] Statistical properties of substructures around MW-size halos and their implications for the formation of stellar streams
78 Masanori Nakamura 中村雅徳 ASIAA
[Oral Presentation] Modeling Parabolic Jets from the Spinning Black Hole
79 David Ni 倪其良 Direxion Technology
[Oral Presentation] Formation of hierarchical stellar systems modeled by Momentum on Complex plane in conjunction with Nonlinear Relativity
80 Takashi Okamoto Hokkaido University
[Oral Presentation] Metal enrichment of simulated galaxies
Top
81 Po-Sheng Ou 歐柏昇 ASIAA / NTU
[Oral Presentation] 1D Simulations of Stellar Mass Loss with the MESA Code
82 Hsing-Po Pan 潘星伯 NCKU
83 Kuo-Chuan Pan 潘國全 National Tsing Hua University
[Oral Presentation] Multi-messenger Signals from Stellar-mass Black Hole Formation
84 Luciano Rezzolla Goethe University Frankfurt am Main, Germany
[Oral Presentation] Binary neutron stars: Einstein's richest laboratory
85 Paul Ricker University of Illinois
[Oral Presentation] Common Envelope Evolution of Massive Binaries
86 Soonyoung Roh UNIST
[Oral Presentation] Turbulence and Magnetic fields in Galaxy Clusters: a Simulation Study
87 Boris Rybakin SRISA RAS, Moscow State University M.V.Lomonosov
[Oral Presentation] Mathematical modeling of the formation of dense clumps in the collisions of molecular clouds
88 Dongsu Ryu UNIST
[Oral Presentation] Shock Waves and their Roles in Astrophysical Turbulence
89 Motoyuki Saijo Waseda University, Japan
[Oral Presentation] Recent understanding of low T/W dynamical instabilities in differentially rotating stars
90 Hsi-Yu Schive 薛熙于 Institute of Astrophysics, National Taiwan University
[Oral Presentation] GAMER-2: GPU-accelerated Adaptive Mesh Refinement
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91 Yuichiro Sekiguchi Toho University
[Oral Presentation] Properties of the dynamical ejecta in binary neutron star merger and r-process nucleosynthesis
92 Hsien Shang 尚賢 ASIAA
93 Chopin Soo National Cheng Kung University
94 Keisuke Sugiura 杉浦 圭祐 Nagoya University, Graduate School of Science
[Oral Presentation] Clarification of Deformation Process of Asteroidal Shapes Through Impact Simulations: Constraint on Collisional History of Large Asteroids
95 Bing Sun 孙兵 Department of Astronomy, Beijing Normal University
96 Scott Suriano The University of Tokyo
[Oral Presentation] The formation of rings and gaps in magnetized wind-launching disks
97 Ronald Taam Northwestern University
98 Satoshi Tanaka 田中 賢 Center for Computational Sciences, University of Tsukuba
[Oral Presentation] Effect of recombination radiation in the formation of first stars
99 Toshiyuki Tanaka 田中 俊行 Nagoya university, Japan
[Oral Presentation] The Impact of Radiative Feedback on The 21-cm Signature around The First Stars
100 Ataru Tanikawa 谷川衝 The University of Tokyo
[Oral Presentation] Numerical Study of White Dwarf Thermonucler Explosions Induced by Tidal Disruption Events
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101 Yong Tian 田雍 Institute of Astronomy, National Central University
102 Kengo Tomida 富田 賢吾 Osaka University / Princeton University
[Oral Presentation] Athena++: a New MHD Simulation Code with Adaptive Mesh Refinement
103 Takuma Tomiyoshi Chiba University
[Poster] 3D-MHD Simulations of Prominences Formation in Rotating Disk
104 Alessandro Trani The University ofTokyo
[Oral Presentation] TSUNAMI: a fast and accurate N-body code for planetary and black hole dynamics
105 Chung Chin Tsai 蔡崇欽 Department of Physics, National Cheng-Kung University
106 Sung-Han Tsai 蔡松翰 ASIAA/NCU
[Oral Presentation] Statistical properties of interacting binary stars with MESA
107 Weiling Tseng 曾瑋玲 Department of Earth Sciences, NTNU
108 Inoue Tsuyoshi 井上剛志 Nagoya University
[Oral Presentation] Bell-Instability-Mediated Spectral Modulation of Gamma Rays from a Supernova Remnant Interacting with Molecular Cloud
109 Koji Uryu 瓜生 康史 Department of Physics, University of the Ryukyus
[Oral Presentation] COCAL: initial data code for numerical relativity
110 Miikka Väisälä 韋米卡 Academia Sinica, Institute of Astronomy and Astrophysics
[Oral Presentation] Astaroth: Accelerating high-order finite-difference hydrodynamics with GPUs
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111 Daw-Wei Wang 王道維 National Tsing Hua University
112 Huiyuan Wang 王慧元 University of Science and Technology of China
113 Haruka Washinoue The University of Tokyo
[Oral Presentation] The Heating of Coronal Loops and X-ray Emission in Low/Zero-metal Stars
114 Tak Pong Woo 胡德邦 Department of Physics, National Taiwan University
115 Meng-Ru Wu 吳孟儒 Institute of Physics, Academia Sinica
[Oral Presentation] r-process nucleosynthesis and kilonovae
116 Toshinori Yamauchi The University of Tokyo
[Oral Presentation] Large-scale parameter search of stellar merger simulations for refinement of intermediate mass black holes formation model
117 I-Ching Yang 楊義清 Department of Applied Science, National Taitung University
118 Yi Yang NCKU
119 tseng Yao-huan ASIAA
120 Chien-Chang Yen 嚴健彰 Fu Jen Catholic University
[Oral Presentation] A direct method for self-gravitational forces on 2D gaseous disks
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121 Hwei-Jang Yo 游輝樟 Department of Physics, National Cheng-Kung University
122 Kohji Yoshikawa 吉川耕司 Center for Computational Sciences, University of Tsukuba
[Oral Presentation] Vlasov-Poisson simulations of cosmic neutrinos in the large-scale structure formation
123 Hoi-Lai Yu 余海禮 Institute of Physics, Academia Sinica
124 KA HO Yuen University of Wisconsin-Madison
[Oral Presentation] Tracing 3D B-field directions and strengths through the Velocity Gradient Technique: Review and prospect
125 Shuai Zha 查帥 the Chinese University of Hong Kong
[Oral Presentation] Hydrodynamic Simulation of Dark Matter Admixed Accretion-Induced Collapse: Gravitational-wave Signals
126 Hong Zhang 張弘 National Taiwan Normal University
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