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.
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Publication: https://arxiv.org/pdf/2208.11996.pdf
Presenters
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Agnieszka M Sorensen
University of Washington
Authors
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Agnieszka M Sorensen
University of Washington
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Dmytro Oliinychenko
N/A
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Volker Koch
Lawrence Berkeley National Laboratory
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Larry D McLerran
University of Washington