MICRA2023: microphysics in computational relativistic astrophysics

Speaker List

• Ryuichiro Akaho (Waseda University)
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    Systematic Study of Fast and Collisional Neutrino Flavor Instabilities in Core-collapse Supernovae with Boltzmann Neutrino Transport

• Haakon Andresen (Stockholm University)
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    Core-Collapse Supernovae: Current Status, Open Questions, and Multi-messenger Prospects

• Debades Bandyopadhyay (Aliah University, Newtown Kolkata - 700160)
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    Equations of State for Supernova and Binary Neutron Star Merger Simulations

• Brandon Barker (Michigan State University)
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    On using Modern Core Collapse Supernova Models to Interpret Observations

• Sebastiano Bernuzzi (FSU Jena)
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    Impact of microphysics in neutron star merger's remnant simulations

• Aurore Betranhandy (Max Planck for gravitational astrophysics)
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    Impact of improved pair-processes transport on the PNS cooling in 2D CCSN simulations

• Mikhail Beznogov (National Institute for R&D in Physics and Nuclear Engineering (IFIN-HH))
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    Bayesian inference of the dense matter equation of state within relativistic mean-field framework

• Bhaskar Biswas (Hamburg University)
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    Multimessenger inference of neutron star equation of state and gravity

• Sebastian Blacker (TU Darmstadt)
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    Thermal behavior as indicator for hyperons in binary neutron star merger remnants

• Luca Boccioli (University of Notre Dame)
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    A quantitative criterion to predict the explodability of core-collapse supernovae: the role of the Si/O interface

• Pablo Bosch (GRAPPA - University of Amsterdam)
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    Multi-messenger Signals from Magnetized Post-Merger Remnants

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    Multi-messenger Signals from Magnetized Post-Merger Remnants

• Alessandro Camilletti (University of Trento)
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    Dynamics and thermodynamics of accretion discs from numerical relativity simulations of neutron star mergers

• Patrick Chi-Kit Cheong (University of New Hampshire)
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    General relativistic multi-group radiation transport simulations of stellar collapses

• Leonardo Chiesa (Università degli Studi di Trento)
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    Nucleosynthesis of light and iron group elements in the ejecta of binary neutron star mergers

• Constantinos Constantinou (INFN/TIFPA)
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    First-order nucleon-to-quark phase transition: Thermodynamically-consistent constructions other than Maxwell and Gibbs.

• William Cook (Friedrich-Schiller-Universität Jena)
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    GRMHD simulations with GR-Athena++

• Harish Chandra Das (Institute of Physics, Bhubaneswar, India)
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    Dark matter effects on the equation of state and the properties of neutron star

• Coleman Dean (University of Alberta)
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    Dynamics of collapsar disk outflow

• Samuel Dunham (Vanderbilt University)
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    A Parametric Study of the SASI Comparing General Relativistic and Non-Relativistic Treatments

• Oliver Eggenberger Andersen (Stockholm University)
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    Explosive Failed Supernovae

• Eirik Endeve (Oak Ridge National Laboratory)
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    A new neutrino transport module available in Flash-X

• Jacob Fields (The Pennsylvania State University)
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    Thermal Effects in Binary Neutron Star Mergers

• Carl Fields (Los Alamos National Laboratory)
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    The Impact of Nuclear Reaction Rate Uncertainties on Progenitors of Core-Collapse Supernovae

• Carla Frohlich (North Carolina State University, United States)
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    Concluding Remarks

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    intro

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    Introduction

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    Networking

• Bruno Giacomazzo (University of Milano)
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    Binary Neutron Star Mergers with Spritz

• Mariam Gogilashvili (Florida State University, Los Alamos National Laboratory)
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    Predicting Which Massive Stars Explode

• Federico Guercilena (TIFPA - INFN (Trento))
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    The influence of trapped neutrinos on the collapse of BNS merger remnants

• Mirco Guerrini (University of Ferrara)
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    First-order transitions at finite temperature

• Goni Halevi
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    The stellar progenitors of long-duration gamma-ray bursts.

• Peter Hammond (NP3M, Pennsylvania State University)
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    Supplementing BNS Simulations with Artificial Neural Networks

• Kai Hebeler (TU Darmstadt)
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    Nuclear EOS for general proton fractions and temperature based on chiral EFT interactions

• Maximilian Jacobi (TU Darmstadt)
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    Nuclear matter properties in neutron star mergers

• Noshad Khosravi Largani (University of Wroclaw)
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    Constraining the onset density for the QCD phase transition with the supernova neutrino signal

• Kelsey Lund
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    TBD

• Fabio Magistrelli (Theoretisch-Physikalisches Institut, Friedrich-Schiller Universitat Jena)
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    Self-consistent evolution of post-merger ejecta: light curves and nucleosynthesis yields

• Gail McLaughlin (North Carolina State University)
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    Neutrino Flavor Transformation in Neutron Star Mergers

• Jonah Miller (Los Alamos National Laboratory)
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    Impact of full neutrino transport in the zoo of post-merger remnants

• Masamitsu Mori (National Astronomical Observatory of Japan)
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    Long term simulation of supernovae for multi-messenger astronomy

• Kanji Mori (National Astronomical Observatory of Japan)
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    Multi-messenger signals of heavy axionlike particles in core-collapse supernovae

• Jeremiah Murphy (Florida State University)
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    Presentation

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    The Progenitor of the Vela Pulsar was Likely a Binary Merger

• Hiroki Nagakura (National Astronomical Observatory of Japan)
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    Neutrino kinetics in core-collapse supernova

• Gerard Navo (TU Darmstadt)
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    CCSN simulations with reduced nucleosynthesis networks

• Anna Neuweiler
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    Kilonova from different points of view: Combining 3D radiative transfer and numerical-relativity simulations

• harry ho-yin NG (Institute for Theoretical Physics, Goethe-Universität Frankfurt)
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    Long-term simulations of Binary neutron star postmerger

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    WeakHub

• Evan O'Connor (Stockholm University, Sweden)
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    Concluding Remarks

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    Introduction

• Micaela Oertel (LUTH-CNRS/Observatoire de Paris)
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    Neutrino interactions in dense and hot matter

• Nils Paar (Faculty of Science University of Zagreb)
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    Stellar weak interaction processes at finite temperature in the relativistic energy density functional theory

• Michael Pajkos (Caltech)
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    Relativistic Capabilities of Core-collapse Supernova Simulations in SpECTRE and Flash

• Albino Perego (University of Trento, Italy)
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    Concluding Remarks

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    Introduction

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    Nucleosynthesis of light and iron group elements in the ejecta of binary neutron star mergers

• Adriana R. Raduta (IFIN-HH, Bucharest)
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    Bayesian inference of the dense matter equation of state built within mean field models

• Moritz Reichert (Universitat de Valencia)
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    The nucleosynthesis of MR-SNe with WinNet

• Giacomo Ricigliano (TU Darmstadt)
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    Impact of nuclear matter properties on the nucleosynthesis and the kilonova from binary neutron star merger ejecta

• Stephan Rosswog
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    Job applications

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    Neutron star mergers with the Lagrangian Numerical Relativity code SPHINCS_BSSN

• Swapnil Shankar (API, University of Amsterdam)
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    Long term simulations of jet-driven core-collapse supernovae on GPUs

• Daniel Siegel
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    Fellowships

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    Jets from neutron-star merger remnants and implications for kilonovae

• Rebecca Surman (University of Notre Dame)
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    Nuclear physics of r-process observables

• Konrad Topolski (Goethe University Frankfurt)
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    Quasi-universal relations of gravitational signal from binary neutron star mergers

• Benjamin Wehmeyer (Konkoly Obs & Univ Hertfordshire)
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    Galactic chemical Evolution with short lived radioactive isotopes

• Liiyung Yeow (The Chinese University of Hong Kong)
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    The impact of different Riemann solvers in neutron star and core-collapse simulations