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    Impact of effective nucleon mass and multineutron states on the equation of state for core-collapse supernovae

    Tatsuya Matsuki

    Shun Furusawa

    Kohsuke Sumiyoshi

    Hong Shen

    Katsuhiko Suzuki

    Phys. Rev. C 114, 025805 – Published 21 August, 2026

    DOI: https://doi.org/10.1103/hxcx-f9sy

    Abstract

    In this study, we investigate the impact of the effective nucleon mass and the existence of the dineutron and the tetraneutron on the thermodynamic properties and nuclear composition by constructing new equations of state. Our results indicate that the model with a larger effective nucleon mass slightly alters the nuclear composition in neutron-rich environments primarily due to differences in the symmetry energy: the mass fractions of unbound neutrons, protons, and heavy nuclei increase. The impact on the thermodynamic properties is negligible, except for the chemical potentials. On the other hand, multineutron states become prominent at high densities in neutron-rich environments, leading to a substantial reduction in the unbound neutron fraction. This depletion lowers the chemical potential of unbound neutrons, which in turn reduces the abundance of neutron-rich nuclei. Consequently, the number of unbound protons increases, leading to a corresponding rise in proton chemical potential. These shifts in chemical potentials promote the formation of heavy nuclei with larger mass and proton numbers. Ultimately, this compositional shift results in a lower free energy, primarily driven by the emergence of these heavy nuclei.

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