Parallel Session Presentation List (Final) Namsan Halls are at 1st floor !!
Room a | Room c | Room d | Room e | Room f | ||
Namsan Hall AB | Namsan Hall C | Namsan Hall D | Namsan Hall E | Namsan Hall F | ||
July 3 (Mon) | Pa1 | A4 | D1 | A1 | A2,D2 | C1 |
Pa2 | A4 | A3 | C2 | E2 | F1 | |
July 4 (Tue) | Pa3 | C3 | E5 | B2 | E4,E1 | A6 |
Pa4 | C3 | E5 | B2 | D3,D4 | B1,G | |
July 6 (Thu) | Pa5 | C3 | E6 | A5 | E7 | B3 |
Pa6 | E6 | A5 | C5 | C4 |
First Name | Middle Name | Last Name | Affiliation | Talk Title | date | time | ID |
A1. General relativity: Theory and Mathematical developments: (Pa1-d, Monday) | Chair: Hyeong-Chan Kim | Pa1-d | |||||
Hyeong-Chan | Kim | Korea National University of Transportation | Steady heat conduction in general relativity | 3 | 14:00-14:20 | Pa1-d1 | |
Sinya | Aoki | Yukawa Institute for Theoretical Physics, Kyoto University | Energy (non-)conservation and a conserved charge in general relativity | 3 | 14:20-14:40 | Pa1-d2 | |
Xiaoning | Wu | Academy of Mathematics and System Science, CAS | On Uniqueness of electro-vacuum static spacetime | 3 | 14:40-15:00 | Pa1-d3 | |
Supragyan | Priyadarshinee | NIT Rourkela, Sundergarh, Odisha, India | Analytic topological hairy dyonic black holes and thermodynamics | 3 | 15:00-15:15 | Pa1-d4 | |
Asta | Heinesen | ENS de Lyon | Dimming of light in general relativity: On the possible emergence of dark energy effects in space-times with ordinary matter | 3 | 15:15-15:30 | Pa1-d5 | |
Dan-Dan | Lian | Sun Yat-sen University | Birefringence of wave packets with angular momentum in gravity | 3 | 15:30-15:45 | Pa1-d6 | |
Yasutaka | Koga | Nagoya University | Photon sphere and shadow evolution in a dynamical black hole spacetime | 3 | 15:45-16:00 | Pa1-d7 | |
A2. Exact solutions: (Pa1-e, Monday) | Chair: Seokcheon Lee | Pa1-e | |||||
Muhammad | Sharif | The University of Lahore | Cosmological Solutions in Extended Theory of Gravity | 3 | 14:00-14:20 | Pa1-e1 | |
Wei-Chen | Lin | Pusan National University | Trouble with the Penrose diagram in spacetimes connected via a spacelike thin shell | 3 | 14:20-14:40 | Pa1-e2 | |
Yeongji | Kim | Konkuk University | Ernst equation in a complete Hamiltonian reduction and exact solutions | 3 | 14:40-14:50 | Pa1-e3 | |
A3. Alternative theory of gravity: (Pa2-c, Monday) | Chair: Jongping Hsu | Pa2-c | |||||
Yu-Xiao | Liu | Lanzhou University | Resonant Kaluza-Klein modes and quasinormal modes on brane | 3 | 16:30-16:50 | Pa2-c1 | |
Shaoqi | Hou | Wuhan University | Gravitational wave memory effects in modified theories of gravity | 3 | 16:50-17:10 | Pa2-c2 | |
Hiroki | Matsui | Yukawa Institute for Theoretical Physics, Kyoto University | DeWitt boundary condition requires Ho\v{r}ava-Lifshitz quantum gravity | 3 | 17:10-17:30 | Pa2-c3 | |
Zheng-Quan | Cui | Sun Yat-Sen University | Spinor Walls in Five-Dimensional Warped Spacetime | 3 | 17:30-17:50 | Pa2-c4 | |
Hongchao | Zhang | Zhejiang University of Technology | Cosmological Constant, Inflaton, and Dark Matter Occurred Naturally from the Duplex Higgs Mechanism for Poincare Gauge Gravity | 3 | 17:50-18:10 | Pa2-c5 | |
Jongping | Hsu | University of Massachusetts Dartmouth | Quantum Yang-Mills Gravity, Feynman-Dyson Rules and Tests | 3 | 18:10-18:30 | Pa2-c6 | |
A4. Modified gravity: (Pa1-a, Monday) | Chair: Yun Soo Myung | Pa1-a | |||||
Boris | Latosh | Center for Theoretical Physics of the Universe, Institute for Basic Science | Scalar-Tensor Gravity at the First Loop | 3 | 14:00-14:25 | Pa1-a1 | |
Avik | De | Universiti Tunku Abdul Rahman | Symmetric teleparallel theory of gravity and its extensions | 3 | 14:25-14:50 | Pa1-a2 | |
Gansukh | Tumurtushaa | Jeju National University | The reheating constraints to natural inflation in Horndeski gravity | 3 | 14:50-15:15 | Pa1-a3 | |
Saikat | Chakraborty | The Institute for Fundamental Study "The Tah Poe Academia Institute", Naresuan University | A comprehensive phase space analysis of the Hu-Sawicki $f(R)$ model | 3 | 15:15-15:40 | Pa1-a4 | |
Arpan | Kar | Center for Quantum Spacetime (CQUeST), Sogang University | WIMPs in Dilatonic Einstein Gauss-Bonnet Cosmology | 3 | 15:40-16:00 | Pa1-a5 | |
A4. Modified gravity: (Pa2-a, Monday) | Chair: Arpan Kar | Pa2-a | |||||
Hocheol | Lee | Sogang University | Cosmology in Double Field Theory | 3 | 16:30-16:45 | Pa2-a1 | |
Dipayan | Mukherjee | Indian Institute of Science Education and Research Mohali | Dual descriptions of late-time cosmology: Bouncing and collapsing Jordan frames | 3 | 16:45-17:00 | Pa2-a2 | |
Kota | Numajiri | Nagoya University | Revisiting TOV Problems in F(R) Gravity | 3 | 17:00-17:15 | Pa2-a3 | |
Tomoya | Tachinami | Hirosaki University | Non-relativistic stellar structure in generic linear massive gravity | 3 | 17:15-17:30 | Pa2-a4 | |
Sojeong | Jung | Sogang University | Thermodynamic phase transitions of the Schwarzschild AdS black hole with the modified Tolman temperature | 3 | 17:30-17:45 | Pa2-a5 | |
Frederic | Lassiaille | FL research | Relativity in motion: long version | 3 | 17:45-18:00 | Pa2-a6 | |
Naoki | Yoshioka | Hiroshima University | Cartan modified gravity and reheating of universe. | 3 | 18:00-18:15 | Pa2-a7 | |
A5. Numerical Relativity: (Pa5-d, Thursday) | Chair: Jinho Kim | Pa5-d | |||||
Chulmoon | Yoo | Nagoya Univ. | Simulation of PBH formation | 6 | 14:00-14:20 | Pa5-d1 | |
Zhoujian | Cao | Chinese Academy of Sciences | Compact Binary object Coalescence along eccentric orbit---From Template to Science | 6 | 14:20-14:40 | Pa5-d2 | |
Yeong-Bok | Bae | Institute for Basic Science | Hyperbolic encounter of two black holes | 6 | 14:40-15:00 | Pa5-d3 | |
Young-Hwan | Hyun | KASI | Imprints of the Strong Gravity Regime in Black Hole Encounters: Insights from Numerical Simulations | 6 | 15:00-15:20 | Pa5-d4 | |
Gungwon | Kang | Chung-Ang University | 3PM EOB Hamiltonian and its numerical test by scattering angles of encountering black holes | 6 | 15:20-15:40 | Pa5-d5 | |
A5. Numerical Relativity: (Pa6-d, Thursday) | Chair: Yeong-Bok Bae | Pa6-d | |||||
Jinho | Kim | Korea Astronomy and Space Science Institute | Relativistic hydrodynamics and its application with AMR | 6 | 16:30-16:50 | Pa6-d1 | |
Ji-hoon | Kim | Seoul National University | How Including New Physics Changes The Evolution of Massive Black Holes In Simulations: Perspectives in the Era of High-resolution Simulations | 6 | 16:50-17:10 | Pa6-d2 | |
Mageshwaran | Tamilan | Chungbuk National University, South Korea | General relativistic advection-dominant accretion disk model in tidal disruption events | 6 | 17:10-17:30 | Pa6-d3 | |
Jeongbhin | Seo | UNIST | Generation of Ultra-High Energy Cosmic Rays at Radio Galaxy Jets | 6 | 17:30-17:50 | Pa6-d4 | |
Shalabh | Gautam | ICTS, Bengaluru | Spherical Einstein Field Equations on Hyperboloidal Slices | 6 | 17:50-18:10 | Pa6-d5 | |
A6. Gravitational waves-Theory: (Pa3-f, Tuesday) | Chair: Jinn-Ouk Gong | Pa3-f | |||||
Karan | Fernandes | National Taiwan Normal University | Gravitational wave observables from subleading soft factors | 4 | 14:00-14:15 | Pa3-f1 | |
Avani | Vikrambhai | Patel | National Taiwan Normal University | Chaotic Orbits in Effective One Body Formulation | 4 | 14:15-14:30 | Pa3-f2 |
Qiliang | Zhao | Sun Yat-sen University | Conformal gravitational waves and their symmetries | 4 | 14:30-14:45 | Pa3-f3 | |
Zi-Yan | Yuwen | Institute of Theoretical Physics,Chinese Academy of Sciences | Hydrodynamic sound shell model | 4 | 14:45-15:00 | Pa3-f4 | |
Shao-Jiang | Wang | Institute of Theoretical Physics, Chinese Academy of Sciences | Hydrodynamic perspective of cosmological first-order phase transitions | 4 | 15:00-15:15 | Pa3-f5 | |
Tie-Jun | Gao | Xidian University | double-inflection-point inflation and gravitational waves | 4 | 15:15-15:30 | Pa3-f6 | |
Chao | Chen | HKUST | Growth of curvature perturbations in non-minimal curvaton scenario | 4 | 15:30-15:45 | Pa3-f7 | |
B1. Quantum physics in curved spacetime: (Pa4-f, Tuesday) | Chair: Shih-Yuin Lin | Pa4-f | |||||
Dong-han | Yeom | Pusan National University | Yang-Mills black holes and end of black hole evaporation | 4 | 16:30-16:50 | Pa4-f1 | |
Shih-Yuin | Lin | National Changhua University of Education | Relativistic particle wavepacket in quantum electromagnetic fields: Quantum coherence and the Unruh effect | 4 | 16:50-17:10 | Pa4-f2 | |
B2. Stringy gravity and AdS/CFT: (Pa3-d, Tuesday) | Chair: Bin Chen | Pa3-d | |||||
Wei | Song | Tsinghua University | The TsT/TTbar correspondence | 4 | 14:00-14:20 | Pa3-d1 | |
Jie-qiang | Wu | Institute of Theoretical Physics, Chinese Academy of Sciences | A Geodesic Network in Classical $AdS_3$ Gravity from the Entanglement Wedge Cross Section | 4 | 14:20-14:40 | Pa3-d2 | |
Cheng | Peng | UCAS, KITS | Spacetime covariant disordered field theories | 4 | 14:40-15:00 | Pa3-d3 | |
Yang | Zhou | Fudan U. | Defect Localized Entropy and Holography | 4 | 15:00-15:20 | Pa3-d4 | |
Run-Qiu | Yang | Tianjin University | On holographic time-like entanglement entropy | 4 | 15:20-15:35 | Pa3-d5 | |
Chanyong | Park | GIST | Holographic two-point functions in a disorder system | 4 | 15:35-15:50 | Pa3-d6 | |
Hao-Tian | Sun | Institute of Theoretical Physics, Chinese Academy of Sciences | Breaking rotations without violating the KSS viscosity bound | 4 | 15:50-15:55 | Pa3-d7 | |
Yuping | An | Institute of Theoretical Physics, Chinese Academy of Sciences | Dynamical Instability of Holographic Two-component Superfluids Interface | 4 | 15:55-16:00 | Pa3-d8 | |
B2. Stringy gravity and AdS/CFT: (Pa4-d, Tuesday) | Chair: Wei Song | Pa4-d | |||||
Bin | Chen | Peking University | On higher-dimensional Carrollian field theory | 4 | 16:30-16:50 | Pa4-d1 | |
Song | He | Jilin University | Pseudo-entropy in 2d CFTs | 4 | 16:50-17:10 | Pa4-d2 | |
Jiang | Long | Huazhong University of Science and Technology | Boundary theory in asymptotically flat spacetime | 4 | 17:10-17:30 | Pa4-d3 | |
XianHui | Ge | Department of Physics, Shanghai University | Matching partition functions of deformed JT gravity and cSYK model | 4 | 17:30-17:45 | Pa4-d4 | |
Wontae | Kim | Sogang University | Temperatures in quantum black holes | 4 | 17:45-18:00 | Pa4-d5 | |
Arpita | Mitra | POSTECH | Soft Theorems in AdS spacetime | 4 | 18:00-18:15 | Pa4-d6 | |
Jun-Kun | Zhao | ITP, CAS | Quantum Critical Magnetocaloric Effect in Holography | 4 | 18:15-18:30 | Pa4-d7 | |
B3. Other topics on Quantum gravity: (Pa5-f, Thursday) | Chair: Pengming Zhang | Pa5-f | |||||
Eric | Bergshoeff | University of Groningen | Carroll Symmetries for Particles, Strings and Gravity | 6 | 14:00-14:20 | Pa5-f1 | |
Glenn | Barnich | Université libre de Bruxelles | Geometric actions in gravity | 6 | 14:20-14:40 | Pa5-f2 | |
Hoi Lai | Yu | Institute of Physics, Academia Sinica, Taiwan | Intrinsic Time Geometrodynamics | 6 | 14:40-15:00 | Pa5-f3 | |
Loïc | Marsot | Sun Yat-sen University | Non-trivial effective null dynamics from extended Carroll symmetries | 6 | 15:00-15:20 | Pa5-f4 | |
Pengming | Zhang | Sun Yat-sen University | Sturm–Liouville equation and Carroll symmetry of plane gravitational wave | 6 | 15:20-15:40 | Pa5-f5 | |
C1. Relativistic Astrophysics: (Pa1-f, Monday) | Chair: Medeu Abishev | Pa1-f | |||||
Nurzada | Beissen | al Farabi Kazakh national university | Application of GBT theorem for Gravitational deflection of light by Compact Objects | 3 | 14:00-14:25 | Pa1-f1 | |
Medeu | Abishev | Al Farabi Kazakh National university | Nonlinear Vacuum Electrodynamic effects on magnetars | 3 | 14:25-14:50 | Pa1-f2 | |
Michail | Chabanov | Goethe University Frankfurt | Crustal magnetic fields do not lead to large magnetic-field amplifications in binary neutron-star mergers | 3 | 14:50-15:15 | Pa1-f3 | |
Myeonghwan | Oh | Kyungpook National University | Accelerated protons produced by magnetic Penrose process in Sgr A* | 3 | 15:15-15:35 | Pa1-f4 | |
C2. Neutron stars & compact objects: (Pa2-d, Monday) | Chair: Jin Young Kim | Pa2-d | |||||
Naresh | Kumar | Patra | BITS Pilani K K Birla Goa Campus, NH-B, South Goa, Goa, Pin-757040 | Systematic analysis of the impacts of symmetry energy parameters on neutron star properties | 3 | 16:30-16:45 | Pa2-d1 |
Muhammad | Zubair | COMSATS University Islamabad, Lahore Campus, Lahore Pakistan | Ultracompact stars in the light of minimal geometric deformation | 3 | 16:45-17:00 | Pa2-d2 | |
Sagnik | Chatterjee | Indian Institute of Science Education and Research Bhopal | Analyzing the speed of sound in neutron stars with machine learning | 3 | 17:00-17:15 | Pa2-d3 | |
Márcio | Ferreira | University of Coimbra | Quark matter in neutron stars | 3 | 17:15-17:30 | Pa2-d4 | |
Yasufumi | Kojima | Hiroshima University | Crustal deformation and fracture by Hall evolution of magnetic field in strongly magnetized stars | 3 | 17:30-17:45 | Pa2-d5 | |
Tursynbek | Izmukhanovich | Yernazarov | al-Farabi Kazakh National University | Nonlinear electrodynamical lensing of electromagnetic waves on the dipole magnetic field of the magnetar. | 3 | 17:45-18:00 | Pa2-d6 |
Yat To | Tang | The Chinese University of Hong Kong | Oscillations and tidal deformations of crystallized white dwarfs | 3 | 18:00-18:15 | Pa2-d7 | |
Jin Young | Kim | Kunsan National University | Light bending by charged black hole and magnetar in the generalized Born-Infeld nonlinear electrodynamics | 3 | 18:15-18:30 | Pa2-d8 | |
C3. Black hole: (Pa3-a, Tuesday) | Chair: Wonwoo Lee | Pa3-a | |||||
Li | Li | Institute of Theoretical Physics, Chinese Academy of Sciences | Probing the structure inside the black hole event horizon | 4 | 14:00-14:20 | Pa3-a1 | |
Zahid | Zakir | Centre for Theoretical Physics and Astrophysics | Metrics with irreducible mass leading to a correct parameter dependence of gravitational effects around charged and rotating compact objects | 4 | 14:20-14:40 | Pa3-a2 | |
Sijie | Gao | Beijing Normal University | General mass formula for charged Kerr-AdS black holes | 4 | 14:40-15:00 | Pa3-a3 | |
Jorge | G. Valcarcel | Tokyo Institute of Technology | New black hole solutions with a dynamical traceless nonmetricity tensor in Metric-Affine Gravity | 4 | 15:00-15:20 | Pa3-a4 | |
Abbas | Mohamed | Sherif | Jeju National University | Thermodynamics from conformal Killing vector in the charged Vaidya metric | 4 | 15:20-15:40 | Pa3-a5 |
C3. Black hole: (Pa4-a, Tuesday) | Chair: Sijie Gao | Pa4-a | |||||
Xiao Yan | Chew | Jiangsu University of Science and Technology | Scalar Hairy Black Holes with Asymmetric Potential | 4 | 16:30-16:50 | Pa4-a1 | |
Wonwoo | Lee | CQUeST, Sogang University | Properties of the charged rotating black hole with an anisotropic matter field | 4 | 16:50-17:10 | Pa4-a2 | |
Daiki | Saito | Nagoya University | Spins of primordial black holes from fluids with soft equation of state parameters | 4 | 17:10-17:30 | Pa4-a3 | |
Saken | Toktarbay | Al farabi kazakh national university | Diverse External Magnetic Field Configurations Surrounding a Black Hole | 4 | 15:30-15:50 | Pa4-a4 | |
C3. Black hole: (Pa5-a, Thursday) | Chair: Li Li | Pa5-a | |||||
Minyong | Guo | Beijing Normal University | Black hole shadow and inner shadow | 6 | 14:00-14:20 | Pa5-a1 | |
Yosuke | Mizuno | Tsung-Dao Lee Institute, Shanghai Jiao Tong University | Numerical Modeling of the Black Hole Shadow and Relativistic Jets on Horizon Scale | 6 | 14:20-14:40 | Pa5-a2 | |
Torben Christian | Frost | Kavli Institute for Astronomy and Astrophysics at Peking University | Gravitational Lensing in the NUT Spacetime: A Multimessenger Approach | 6 | 14:40-15:00 | Pa5-a3 | |
Hsu-Wen | Chiang | LeCosPA, NTU | Relating photon orbit observable with quasinormal modes in generic axisymmetric stationary spacetime | 6 | 15:00-15:20 | Pa5-a4 | |
Koichiro | Uehara | Nagoya University | Numerical simulation of type II primordial black hole formation | 6 | 15:20-15:40 | Pa5-a5 | |
Albert | Escrivà | Nagoya University | Numerical simulations of vacuum bubbles and their consequences on the PBH scenario | 6 | 15:40-16:00 | Pa5-a6 | |
C4. Wormholes and other massive objects: (Pa6-f, Thursday) | Chair: Wontae Kim | Pa6-f | |||||
Francisco | S.N. | Lobo | Institute of Astrophysics and Space Sciences, University of Lisbon | Modified-gravity wormholes without exotic matter | 6 | 16:30-17:00 | Pa6-f1 |
Sung-Won | Kim | Ewha Womans University | Gravitational waves by a wormhole and wormhole binary system | 6 | 17:00-17:20 | Pa6-f2 | |
Pradyumn | Kumar | Sahoo | BITS-Pilani, Hyderabad Campus | A study on Casimir wormholes | 6 | 17:20-17:40 | Pa6-f3 |
Paul | Bikash | Chandra | University of North Bengal | Emergent Universe from Dynamical wormhole | 6 | 17:40-18:00 | Pa6-f4 |
Keiya | Uemichi | Nagoya University | General solution of 5 dimensional rotating wormhole | 6 | 18:00-18:15 | Pa6-f5 | |
Hyat | Huang | University of Oldenburg | Light Ring behind Wormhole Throat | 6 | 18:15-18:30 | Pa6-f6 | |
Fech Scen | Khoo | University of Oldenburg | Stability of slowly rotating Ellis-Bronnikov wormholes | 6 | 18:30-18:45 | Pa6-f7 | |
C5. Dark Matter: (Pa6-e, Thursday) | Chair: Jaeweon Lee | Pa6-e | |||||
Xing-Yu | Yang | KIAS | Observational phenomena on black hole with dark matter dress | 6 | 16:30-16:45 | Pa6-e1 | |
Hiroki | Kawai | University of Tokyo | An analytic model for the core-halo mass relation in fuzzy dark matter halos | 6 | 16:45-17:00 | Pa6-e2 | |
Tan | Chen | Institute of Theoretical Physics, Chinese Academy of Sciences | Gravitational microlensing by dressed primordial black holes | 6 | 17:00-17:15 | Pa6-e3 | |
Ning | Xie | Sun Yat-sen University | Imprints of ultralight axions on the gravitational wave and pulsar timing measurement | 6 | 17:15-17:30 | Pa6-e4 | |
Junseok | Lee | Tohoku University | The evolution of domain wall network with inflationary fluctuations | 6 | 17:30-17:45 | Pa6-e5 | |
Naoya | Kitajima | Tohoku University | Cosmological production of dark photon dark matter | 6 | 17:45-18:00 | Pa6-e6 | |
Keiko | Nagao | Okayama University of Science | Directional detection of boosted dark matter from direction of the Galactic center | 6 | 18:00-18:15 | Pa6-e7 | |
Yun-Long | Zhang | National Astronomical Observatories, Chinese Academy of Sciences | Pulsar timing residual induced by wideband ultralight dark matter | 6 | 18:15-18:30 | Pa6-c8 | |
D1. Dark Energy: (Pa1-c, Monday) | Chair: Jaeweon Lee | Pa1-c | |||||
Young-Wook | Lee | Yonsei University | Evidence for strong progenitor age bias in supernova cosmology | 3 | 14:00-14:20 | Pa1-c1 | |
Eoin | O Colgain | Atlantic Technological University | Is H0 a constant? | 3 | 14:20-14:40 | Pa1-c2 | |
Jaeweon | Lee | Jungwon univ. | Dark energy from quantum entanglement | 3 | 14:40-15:00 | Pa1-c3 | |
Md | Saddam | Hussain | Indian Institute of Technology Kanpur, India | Dynamics of Interacting Dark Matter Dark Energy | 3 | 15:00-15:20 | Pa1-c4 |
Fei | Qin | Korea Astronomy and Space Science Institute | The Halo Occupation Distribution of HI Galaxies | 3 | 15:20-15:40 | Pa1-c5 | |
D2. Status of Standard cosmology and alternatives: (Pa1-e, Monday) | Chair: Seokcheon Lee | Pa1-e | |||||
Daniele | Gregoris | Jiangsu University of Science and Technology | On the uniqueness of ΛCDM-like evolution for homogeneous and isotropic cosmology in General Relativity | 3 | 14:50-15:10 | Pa1-e4 | |
Seokcheon | Lee | Sungkyunkwan University | Late time acceleration with varying speed of light model | 3 | 15:10-15:30 | Pa1-e5 | |
Minyong | Jung | Seoul National University | Satellite Galaxy Populations In A Cosmological Simulation | 3 | 15:30-15:45 | Pa1-e6 | |
D3. Cosmological dynamics and Fundamental Constants: (Pa4-e, Tuesday) | Chair: Seung Hun Oh | Pa4-e | |||||
Kenmoku | Masakatsu | Nara Women's Universiry | Singularities of Magnetic Monopoles in the Universe | 4 | 16:30-16:50 | Pa4-e1 | |
Jie | Jiang | Pusan National University | Numerical Investigation of Two-Dimensional Fokker-Planck Equation in Inflationary Models: Importance of Slow-Roll Conditions | 4 | 16:50-17:10 | Pa4-e2 | |
D4. Cosmology beyond FLRW-theory and Obs: (Pa4-e, Tuesday) | Chair: Seung Hun Oh | ||||||
Ya-Peng | Hu | Nanjing University of Aeronautics and Astronautics | Thermodynamic equation of state and phase transitions for the spacetime of Friedmann-Robertson-Walker universe | 4 | 17:10-17:30 | Pa4-e3 | |
Vipin | Sudevan | LeCosPA, NTU, Taiwan | A DEEP LATENT VARIABLE MODEL FOR RECOVERING CMB ANISOTROPY MAP OVER LARGE ANGULAR SCALES OF THE SKY | 4 | 17:30-17:50 | Pa4-e4 | |
Ashok | Kumar | Singal | Physical Research Laboratory, Ahmedabad | Discordance of dipole asymmetries seen in large radio surveys (VLASS & RACS) with the Cosmological Principle | 4 | 17:50-18:10 | Pa4-e5 |
E1. Test of gravity: (Pa3-e, Tuesday) | Chair: Myungshin Im | Pa3-e | |||||
Che-Yu | Chen | iTHEMS, RIKEN | Testing black hole eikonal correspondence | 4 | 15:00-15:20 | Pa3-e4 | |
Yun | Hao | University of Massachusetts Dartmouth | Testing Gravitational Violation of Electromagnetic $U_1$ Symmetry: Light Deflection by the Sun and Josephson Effects in Quantum Yang-Mills Gravity | 4 | 15:20-15:40 | Pa3-e5 | |
E2. EHT (Event Horizon Telescope): (Pa2-e, Monday) | Chair: Georgios Paraschos | Pa2-e | |||||
Georgios | Filippos | Paraschos | Max Planck Institute | AGN studies with the EHT and synergies with GR/theory | 3 | 16:30-17:00 | Pa2-e1 |
Dongjin | Kim | MIT | EHT Simulations: A Preview of the Next Decade | 3 | 17:00-17:30 | Pa2-e2 | |
Benjamin | Scott | Prather | Los Alamos National Laboratory | Insights From the First Polarized Images of the Supermassive Black Hole M87* | 3 | 17:30-18:00 | Pa2-e3 |
Ilje | Cho | IAA-CSIC, Spain | Imaging the Black Hole Shadow from the EHT observations | 3 | 18:00-18:30 | Pa2-e4 | |
E4. Multi-Messenger Astrophysics: (Pa3-e, Tuesday) | Chair: Myungshin Im | Pa3-e | |||||
Elahe | Khalouei | Seoul National University | Electromagnetic follow-up of GW | 4 | 14:00-14:20 | Pa3-e1 | |
Surojit | Saha | Institute of Astronomy, National Tsing Hua University, Taiwan | Rapid Generation of Kilonova Light Curves Using Conditional Variational Autoencoder | 4 | 14:20-14:40 | Pa3-e2 | |
Alexei | Sytov | INFN Ferrara Division; Korea Institute of Science and Technology Information (KISTI) | New ideas for dark matter search in dwarf galaxies through direct gamma-ray detection exploiting the acceleration of electromagnetic shower development in oriented crystals | 4 | 14:40-15:00 | Pa3-e3 | |
E5. Gravitational wave detection: (Pa3-c, Tuesday) | Chair: Ho Jung Paik | Pa3-c | |||||
Jianwei | Mei | TianQin Center, Sun Yat-sen University | Science of TianQin | 4 | 14:00-14:25 | Pa3-c1 | |
Yanzheng | Bai | Huazhong University of Science&Technology | Progress of high-precision inertial sensor for TianQin | 4 | 14:25-14:50 | Pa3-c2 | |
Minghui | Du | Institute of Mechanics, Chinese Academy of Science | Constraining Kaluza-Klein extra dimensions with Taiji | 4 | 14:50-15:15 | Pa3-c3 | |
Xinmiao | Zhao | Peking University | Constraining the acceleration of moving binary black holes using gravitational wave | 4 | 15:15-15:40 | Pa3-c4 | |
E5. Gravitational wave detection: (Pa4-c, Tuesday) | Chair: Li Li | Pa4-c | |||||
Ho Jung | Paik | Department of Physics, University of Maryland, College Park, MD | SOGRO in Tetrahedral Configuration for Mid-Frequency Gravitational Waves | 4 | 16:30-17:00 | Pa4-c1 | |
Bian | Institute of Mechanics, Chinese Academy of Sciences | Development of Superconducting Weak Force Sensors for Gravitational Wave Detection | 4 | 17:00-17:25 | Pa4-c2 | ||
Chan | Park | IBS | Detection of gravitational waves by electromagnetic cavity: a review | 4 | 17:25-17:50 | Pa4-c3 | |
E6. LIGO theory and experiment: (Pa5-c, Thursday) | Chair: Chunglee Kim | Pa5-c | |||||
Shinji | Miyoki | ICRR, The University of Tokyo | Overview of the KAGRA commissioning for O4 | 6 | 14:00-14:30 | Pa5-c1 | |
Sungho | Lee | Korea Astronomy and Space Science Institute (KASI) | Development of Gravitational Wave Detection Technology at KASI | 6 | 14:30-14:50 | Pa5-c2 | |
June Gyu | Park | Yonsei university | Lab-Scale Experiment for Laser Interferometer Gravitational Wave Detector | 6 | 14:50-15:10 | Pa5-c3 | |
Daiki | Haba | Tokyo Institute of Technology | Development of a new control method for optical resonators under the influence of non-uniform birefringence | 6 | 15:10-15:30 | Pa5-c4 | |
Seiya | Sasaoka | Tokyo Institute of Technology | Deep Learning for Gravitational Wave Detection and Its Analysis Using Grad-CAM | 6 | 15:30-16:00 | Pa5-c5 | |
E6. LIGO theory and experiment: (Pa6-c, Thursday) | Chair: Hyung Mok Lee | Pa6-c | |||||
Md Arif | Shaikh | Seoul National University | Defining Eccentricity for Gravitational Wave Astronomy | 6 | 16:30-16:50 | Pa6-c1 | |
Soichiro | Morisaki | Institute for Cosmic Ray Research, University of Tokyo | Rapid parameter estimation of binary neutron star merger using reduced order quadrature | 6 | 16:50-17:10 | Pa6-c2 | |
JeongCho | Kim | Seoul National University | Effects of eccentricity and aligned spins in the parameter estimation of CBC inspirals | 6 | 17:10-17:30 | Pa6-c3 | |
E7. LISA theory and experiment: (Pa5-e, Thursday) | Chair: John Conklin | Pa5-e | |||||
Masaki | Ando | University of Tokyo | Space Gravitational-Wave Antenna B-DECIGO and DECIGO | 6 | 14:00-14:20 | Pa5-e1 | |
John | G | Baker | NASA-GSFC | NASA's Contributions to LISA Science and Technology | 6 | 14:20-14:40 | Pa5-e2 |
Ziren | Luo | Chinese Academy of Sciences | The recent status of Taiji program | 6 | 14:40-15:00 | Pa5-e3 | |
Yongho | Lee | AEI Hannover | LISA Phase Measurement System Development and Testing | 6 | 15:00-15:20 | Pa5-e4 | |
Davide | Dal Bosco | University of Trento and INFN/TIFPA | The LISA Gravitational Reference Sensor: technology and challenges | 6 | 15:20-15:40 | Pa5-e5 | |
Veronica | Vazquez-Aceves | The Kavli Institute for Astronomy and Astrophysics, Pekin University | XMRI in the centre of our galaxy, formation mechanisms and the information we can extract from them. | 6 | 15:40-16:00 | Pa5-e6 | |
F1. Education on Astrophysics and Relativity: (Pa2-f, Monday) | Chair: Sung-Won Kim | Pa2-f | |||||
Jongwon | Park | Chonnam National University | Teaching relativity theory to foster scientific literacy | 3 | 16:30-17:00 | Pa2-f1 | |
Wonyong | Park | University of Southampton | Making the relativity curriculum: Recent curriculum reforms in Korea and competing views about physics knowledge | 3 | 17:00-17:20 | Pa2-f2 | |
Ajay | Sharma | Fundamental Physics Society | Re-visiting Einstein’s original derivation of E =mc2 | 3 | 17:20-17:40 | Pa2-f3 | |
Sungmin | Im | Daegu University | Analysis of pre-service physics teachers’ conceptual understanding on special relativity theory | 3 | 17:40-18:00 | Pa2-f4 | |
Dong-han | Yeom | Pusan National University | A heuristic approach to compute the bending of light | 3 | 18:00-18:15 | Pa2-f5 | |
Jin Young | Kim | KARTS | The convergence of astrophysics and modern art after World War II | 3 | 18:15-18:30 | Pa2-f6 | |
G: After-deadline: (Pa4-f, Tuesday) | Chair: Shih-Yuin Lin | Pa4-f | |||||
Tomohiro | Harada | Rikkyo University | The periapsis shift of a quasi-circular orbit in a static spherically symmetric spacetime and the active gravitational mass density | 4 | 17:10-17:30 | Pa4-f3 | |
Si-Jiang | Yang | Lanzhou University | Thermodynamics and weak cosmic cernsorship conjecture for a Kerr-Newman Taub-NUT black hole | 4 | 17:30-17:45 | Pa4-f4 | |
Mahdis | Ghodrati | APCTP | Black hole radiation phase space from 1d higher point of view | 4 | 17:45-18:00 | Pa4-f5 | |
Shao-Jiang | Wang | Institute of Theoretical Physics, Chinese Academy of Sciences | Is there a Hubble-variation tension? | 4 | 18:00-18:20 | Pa4-f6 |