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Dense Nuclear Matter Equation of State from Theory and Experiments

28 octobre 2024 à 1 novembre 2024
IRL-NPA FRIB
Fuseau horaire US/Eastern

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Liste des Contributions

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  1. 29. Registration
    28/10/2024 09:00
  2. 30. Workshop opening & the code of conduct
    28/10/2024 09:15
  3. 31. Discussion of the workshop goals & strategies
    28/10/2024 09:30
  4. 6. Combined Inference from Neutron Stars and Nuclei
    William Newton (Texas A&M University-Commerce)
    28/10/2024 09:45
  5. 7. Equation of state of dense matter: Inference from gravitational waves
    Anthea FANTINA (GANIL ({CNRS}UPR3266))
    28/10/2024 11:00
  6. 8. From nuclei to neutron stars in the unifying framework of energy density functional theory
    Panagiota Papakonstantinou (IBS/IRIS)
    28/10/2024 11:45
  7. 9. The equation of state of symmetric nuclear matter from heavy-ion collisions
    Agnieszka Sorensen (University of Washington)
    28/10/2024 14:00
  8. 10. Heavy-ion collision measurements at early FRIB and a look towards FRIB400
    Kyle Brown (Michigan State University)
    28/10/2024 14:45
  9. 11. From heavy-ion collisions at intermediate energies to the nuclear equation of state in symmetric nuclear matter
    Rohit Kumar
    29/10/2024 09:00
  10. 12. Nuclear equation of state constraints from intermediate energy heavy-ion collisions
    Caterina Ciampi (GANIL)
    29/10/2024 09:30
  11. 13. Constraining the in-medium cross section in transport simulations with Ca+Ni collisions at 140 MeV/nucleon
    Chi Kin Tam (Western Michigan University)
    29/10/2024 10:00
  12. 14. Transport model based on inputs from chiral effective field theory
    Che-Ming Ko (Texas A&M University)
    29/10/2024 12:30
  13. 15. Accessing new observables from heavy-ion collisions at FRIB
    Simone Valdre' (INFN - Sezione di Firenze)
    30/10/2024 09:00
  14. 16. Transport Theory and Correlation Measurements: Coming to Terms on Emission Sources
    Pierre Nzabahimana
    30/10/2024 09:30
  15. 17. Decoding the composition of QCD matter with the polarization of thermal dileptons
    Florian Seck (TU Darmstadt)
    30/10/2024 10:00
  16. 18. Harmonic flow correlations as a precision tool for measuring the nuclear EoS at large baryon densities
    Tom Reichert
    30/10/2024 11:00
  17. 19. Structure in the speed of sound: from neutron stars to heavy-ion collisions
    Nanxi Yao (University of Illinois, Urbana-Champaign)
    30/10/2024 11:30
  18. 21. Reproducible Bayesian Workflows for Model Mixing and Calibration
    Kyle Godbey
    31/10/2024 09:00
  19. 23. Bayesian calibration of the in-medium modification of the light cluster binding energies
    Diego Gruyer (LPC Caen)
    31/10/2024 09:45
  20. 24. From chiral EFT to perturbative QCD: a Bayesian model mixing approach to the dense matter equation of state
    Alexandra Semposki (Ohio University)
    31/10/2024 11:00
  21. 22. Nuclear equation of state from nuclear experiments and neutron star observations
    Pietro Klausner (Université de Normandie - Caen / LPC / Università degli studi di Milano)
    31/10/2024 11:30
  22. 25. Minimizing Emulator Uncertainty
    Oleh Savchuk (Bogolyubov Institute for Theoretical Physics)
    31/10/2024 12:00
  23. 26. Role of CBM-FAIR in Multi-Messenger Pursuit of Dense Matter EOS
    Kshitij Agarwal (Eberhard Karls Universität Tübingen (DE))
    01/11/2024 09:00
  24. 27. Hyperonic phase transitions in dense matter
    Nikolas Cruz Camacho (University of Illinois at Urbana-Champaign)
    01/11/2024 09:30
  25. 28. MUSES – An overview: The nuclear phase diagram puzzle from neutron stars to heavy-ion collisions
    Johannes Jahan (University of Houston)
    01/11/2024 10:00
  26. 20. Intro to chiEFT
    Christian Drischler (Ohio University)