Poster Presentations in the 2nd week
(February 2 - February 6)
[Instruction for poster presenters]
- Sara Azizi (University of Amsterdam)
"A resistive MHD module in the GPU-accelerated GRMHD code GRaM-X"
- Cheuk Nam Chong (The Chinese University of Hong Kong)
"Rotating, Magnetic White Dwarfs as Progenitors of Superluminous Type Ia Supernovae"
- Vincent Ernst (University of Louvain)
"Impact of resonant modes in binary neutron stars on gravitational-wave parameter estimation"
- Joan Fontbuté (Friedrich-Schiller Universität - Jena)
"Gravitational Scattering of two Neutron Stars"
- Ritesh Harshe (Tata Institute of Fundamental Research)
"Search for the Evidence of Lensing in the LIGO-Virgo-KAGRA Observations"
- Javiera Hernández Morales (University of Greifswald)
"Accretion Regimes of Neutrino-Cooled Flows onto Black Holes"
- Yongjia Huang (Purple mountain observatory/ RIKEN)
"Binary Neutron Star Merger as a Probe of Hadron-Quark Transition"
- Giulia Huez (Friedrich-Schiller University Jena)
"Binary neutron stars: multi-messenger analyses to constrain equation of state"
- Krishna Kumar (University of Leeds)
"Dynamics of kink unstable, highly magnetized, static AGN jets and their interaction with winds and disk. "
- Matus Labaj (Masaryk University)
"Accretion and Outflows around Intermediate-Mass Black Holes in Compact Stellar Systems"
- Fabio Magistrelli (Friedrich-Schiller Universitaet Jena)
"Effects of in-situ nuclear networks and atomic opacities in BNSM ejecta modeling"
- Michael Mueller (University of Greifswald)
"Hypermassive neutron stars as GRB central engines"
- Piotr Płonka (Center for Theoretical Physics PAS)
"Three-dimensional GRMHD simulations of jet formation and propagation in self-gravitating collapsing stars"
- Joseph Saji (Polish Academy of Sciences)
"The Origin of Heavy Elements in the Universe: Insights from GRMHD Simulations of Accretion-Disk Outflows"
- Blanka Világos (Stockholm University)
"Towards kilonova modelling in 3D NLTE with ExTraSS"
- Liiyung Yeow (The Chinese University of Hong Kong)
"The impact of different Riemann solvers in neutron star simulations"