Bayesian analysis for constraining the equation of state of asymmetric nuclear matter

ORAL

Abstract

The equation of state of nuclear matter plays a crucial role in understanding the properties of neutron stars and heavy-ion collisions. However, due to the complexities of nuclear interactions, accurately constraining the EoS remains a challenging task. We present results of combining Bayesian analysis of the transport model simulations and the single particle spectra, and particle ratios from the Ca+Ni and Ca+Sn collisions at E/A=56 and 140 MeV performed at the National Superconducting Cyclotron Laboratory.

*This work was supported in part by the U.S. National Science Foundation under Grants PHY-1565546, PHYS-1712832, and PHY-2110218; in part by the U.S. Department of Energy (the Office of Science) under Grant DE-NA0003908;

–

Presenters

  • Zbigniew Chajecki

    • Western Michigan University

Authors

  • Zbigniew Chajecki

    • Western Michigan University

  • Manyee B Tsang

    • Michigan State University

  • William G Lynch

    • Michigan State University

  • Chi-En Teh

    • National Superconducting Cyclotron Laboratory, MSU
    • Facility for Rare Isotope Beams, MSU

  • Chi-Kin Tam

    • Western Michigan University

  • Som N Paneru

    • Michigan State University

  • Kyle W Brown

    • Michigan State University

  • Kuan Zhu

    • Michigan State University

  • Daniele Dell’Aquila

    • UNIVERSITA' DEGLI STUDI DI NAPOLI

  • Chun Yuen Tsang

    • Kent State University

  • Adam K Anthony

    • Michigan State University

  • Om Bhadra Khanal

    • Western Michigan University

  • Justin B Estee

    • Michigan State University

  • Jonathan E Barney

    • Michigan State University

  • Sean R Sweany

    • Michigan State University