The equation of state of dense nuclear matter from heavy-ion collisions

ORAL

Abstract

We use hadronic transport simulations with parametrizable mean-field interactions together with flow data from the STAR experiment at the center-of-mass energies of 3.0 and 4.5 GeV to constrain the equation of state of symmetric nuclear matter through Bayesian analysis. I will discuss the findings in the context of other known constraints from heavy-ion collisions and neutron star studies.

*Support by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Grant No. DE-FG02-00ER41132, is gratefully acknowledged.

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Publication: https://arxiv.org/pdf/2208.11996.pdf

Presenters

  • Agnieszka M Sorensen

    • University of Washington

Authors

  • Agnieszka M Sorensen

    • University of Washington

  • Dmytro Oliinychenko

    • N/A

  • Volker Koch

    • Lawrence Berkeley National Laboratory

  • Larry D McLerran

    • University of Washington