Constraining neutron-proton effective mass splitting through nuclear giant dipole resonance within transport approach

TL;DR

This study uses a transport approach to analyze how the neutron-proton effective mass splitting influences nuclear giant dipole resonance, providing constraints on the isovector effective mass and mass splitting in nuclear matter.

Contribution

It introduces a Bayesian method to constrain the neutron-proton effective mass splitting using giant dipole resonance data within a transport model framework.

Findings

The energy-weighted sum rule $m_1$ is highly sensitive to $m^*_{v,0}$.

The width $ extGamma$ of IVGDR is mainly governed by in-medium nucleon-nucleon cross section.

The neutron-proton effective mass splitting coefficient at saturation density is quantified.

Abstract

Based on the Boltzmann-Uehling-Uhlenbeck equation, we investigate the effects of the isovector nucleon effective mass $m^*_{v,0}$ and the in-medium nucleon-nucleon cross section $\sigma^*$ on the isovector giant dipole resonance~(IVGDR) in $^{208}{\rm Pb}$, employing a set of representative Skyrme energy density functionals. We find that the energy-weighted sum rule $m_1$ of the IVGDR is highly sensitive to $m^{*}_{v,0}$ and only mildly dependent on $\sigma^*$, while the width $\Gamma$ of the IVGDR is primarily governed by $\sigma^*$ with a moderate sensitivity to $m^*_{v,0}$. From a Bayesian analysis of both $m_1$ and $\Gamma$, we infer the isovector effective mass $m^{*}_{v,0}/m$ = $0.731^{+0.027}_{-0.023}$, where $m$ is the bare nucleon mass. Furthermore, by incorporating the isoscalar effective mass $m^*_{s,0}/m = 0.820 \pm 0.030$, extracted from the isoscalar giant quadrupole resonance in $^{208}{\rm Pb}$, the linear neutron-proton effective mass splitting coefficient at saturation density $\rho_0$ is determined to be $\Delta m^*_1 (\rho_0)/m = 0.200 ^{+0.101}_{-0.094}$.