Event Schedule

Dense Nuclear Matter Equation of State from Heavy-Ion Collisions

All time info. is in Pacific Standard Time (UTC -8); please convert accordingly.

Please note: By attending a workshop talk, participants agree to abide by the INT Code of Conduct

Week 1

Monday, December 5, 2022

Start Time Presentation Title Presenter Presenter Organization Format Location Slides
Workshop opening & the INT code of conduct Vincenzo Cirigliano Institute for Nuclear Theory In-person C520
Probing the EOS through HICs and simulations Paweł Danielewicz Michigan State University In-person C520 PDF
The Equation of State of Symmetric Nuclear Matter from Intermediate Energy Heavy-Ion Data Dan Cozma IFIN-HH Virtual C520 PDF
Constraints from the SpiRIT experiment and their implications on nuclear matter equation of state Tommy Tsang Kent State University In-person C520 PDF
COFFEE BREAK
PARALLEL DISCUSSION C421: EOSs for hadronic transport: theory sources (chiEFT, many-body theory, neutron star EOS, ...) and implementation In-person C421
PARALLEL DISCUSSION C520: Experiments and detectors of the future: FAIR, FRIB400, J-PARC, ... In-person C520
LUNCH BREAK
PLENARY DISCUSSION C520
Scalar and vector type momentum-dependent potentials in the relativistic molecular dynamics and the anisotropic flow Yasushi Nara Akita International University Virtual C520 PDF
Harmonic flow correlations as a testing ground for the nuclear EoS Tom Reichert Institut fuer Theoretische Physik Virtual C520 PDF
Enhanced dilepton emission from a phase transition in dense matter Oleh Savchuk Bogolyubov Institute For Theoretical Physics In-person C520 PDF
The EoS of dense nuclear matter from Bayesian analysis of heavy-ion collision data Manjunath Omana Kuttan Frankfurt Institute for Advanced Studies In-person C520 PDF
COFFEE BREAK
PLENARY DISCUSSION: The EOS for hadronic transport: the momentum- and isospin-dependence, strangeness, causality, ... In-person C520

Tuesday, December 6, 2022

Start Time Presentation Title Presenter Presenter Organization Format Location Slides
Collective flow measurements in Gold-Gold collisions at 1.23 AGeV with HADES Behruz Kardan Institut fuer Kernphysik In-person C520 PDF
Proton-cluster correlations at HADES experiment Maria Stefaniak GSI Helmholtz Centre for Heavy Ion Research In-person C520 PDF
STAR: net-proton fluctuations and spectra results from BES-II/FXT Daniel Cebra University of California, Davis In-person C520 PDF
COFFEE BREAK
PARALLEL DISCUSSION C423: Nuclear theory and astrophysics input to the White Paper In-person C423
PARALLEL DISCUSSION C520: Experimental input to the White Paper In-person C520
PARALLEL DISCUSSION C421: Hadronic transport theory input to the White Paper In-person C421
LUNCH BREAK
PLENARY DISCUSSION In-person C520
Two-particle correlations at the BES program Hanna Zbroszczyk Warsaw University of Technology In-person C520 PDF
Reaction Plane Correlated Triangular Flow in Au+Au Collisions at \sqrt{s_{NN}} = 3.0 GeV from STAR Cameron Racz University of California, Riverside In-person C520 PDF
Probing the equation of state of nuclear matter with heavy ion collisions Zbigniew Chajecki Western Michigan University In-person C520 PDF
Deblurring source function from particle correlations in heavy-ion collisions Pierre Nzabahimana FRIB/Michigan State University In-person C520 PDF
COFFEE BREAK
PLENARY DISCUSSION: Experimental signals for the EOS / dense nuclear matter properties vs. theoretical expectations: the pion problem, Lambda potential, meson flow, HBT, ... In-person C520

Wednesday, December 7, 2022

Start Time Presentation Title Presenter Presenter Organization Format Location Slides
Fragmentation mechanisms in heavy-ion collisions and stochastic transport models Maria Colonna INFN-LNS Virtual C520 PDF
Spinodal Enhancement of Light Nuclei Yield Ratio in Relativistic Heavy-Ion Collisions Kaijia Sun Cyclotron Institute Virtual C520 PDF
The influence of light nuclei production and the EOS on flow in low-energy heavy-ion collisions Justin Mohs Institute for Theoretical Physics In-person 520 PDF
COFFEE BREAK
PARALLEL DISCUSSION C520: Neutron star and neutron star mergers theory In-person C520
PARALLEL DISCUSSION C421: Hadronic transport theory needs (momentum-dependent potentials, isospin dependence away from saturation, temperature dependence, ...) In-person C421
LUNCH BREAK
Probing the EoS of dense matter with fluctuation observables in heavy-ion collisions Volodymyr Vovchenko Institute for Nuclear Theory In-person C607 PDF
PLENARY DISCUSSION In-person C607
Resources for diversifying nuclear physics Agnieszka Sorensen Institute for Nuclear Theory In-person C607 PDF
DEIA in nuclear physics: open mic / discussion In-person C607
COFFEE BREAK
PLENARY DISCUSSION: Hadronic transport implementation: initial state, in-medium cross sections, coalescence, fragment formation, fluctuations, ... In-person C607

Thursday, December 8, 2022

Start Time Presentation Title Presenter Presenter Organization Format Location Slides
Characterization of nuclear pasta by alpha shapes method Jorge Lopez University of Texas at El Paso In-person C520 PDF
Net strangeness and isospin fractions in the EOS as probed by protoneutron stars, binary neutron stars mergers, and heavy-ion collisions Veronica Dexheimer Kent State University Virtual C520 PDF
Dense matter EOS and neutron star properties constrained by nuclear experiments and astrophysical observations Rohit Kumar Michigan State University, Michigan In-person C520 PDF
COFFEE BREAK
PARALLEL DISCUSSION C421: Hadronic transport theory needs In-person C421
PARALLEL DISCUSSION C423: Hydrodynamics for neutron stars and high-energy physics In-person C423
PARALLEL DISCUSSION C520: Challenges for theory calculations at high density In-person C520
LUNCH BREAK
PLENARY DISCUSSION In-person C520 PDF
Mapping the binary neutron star merger conditions to heavy-ion collisions with a single EoS Anton Motornenko Frankfurt Institute for Advanced Studies In-person C520 PDF
Heavy-ion collision matter in modified-gravity neutron stars Jose Carlos Jimenez Apaza Institute of Physics In-person C520 PDF
Hybrid equations of state for neutron stars with deltas and hyperons Rajesh Kumar Kent State University In-person C520 PDF
Constraining Nuclear Symmetry Energy from Converting Neutron Star EoS into HI Collisions Nanxi Yao University of Illinois, Urbana-Champaign In-person C520 PDF
COFFEE BREAK
PLENARY DISCUSSION: Global analyses, ... In-person C520

Friday, December 9, 2022

Start Time Presentation Title Presenter Presenter Organization Format Location Slides
Constraining the nuclear EOS with theory, observations, and experiment Ingo Tews Los Alamos National Laboratory Virtual C520 PDF
Current constraints on the neutron star equation of state and non-trivial features in the EoS Débora Mroczek University of Illinois Urbana Champaign In-person C520 PDF
The role of CBM-FAIR in probing dense nuclear matter EOS Kshitij Agarwal Eberhard Karls Universitaet Tuebingen Virtual C520 PDF
COFFEE BREAK
BSQ Hydrodynamics and challenges with a 4D equation of state Christopher Plumberg Pepperdine University Virtual C520 PDF
Cosmic applications of hadron transport Ramona Vogt LLNL / UC Davis Virtual C520 PDF
PLENARY DISCUSSION In-person C520
LUNCH BREAK
WORKSHOP CONCLUSION In-person C520