Charge symmetry breaking effects of $ω$-$ρ^0$ mixing in relativistic mean-field model

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Hauptverfasser: Tanimura, Yusuke, Naito, Tomoya, Sagawa, Hiroyuki, Cheoun, Myung-Ki
Format: Preprint
Veröffentlicht: 2025
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author Tanimura, Yusuke
Naito, Tomoya
Sagawa, Hiroyuki
Cheoun, Myung-Ki
author_facet Tanimura, Yusuke
Naito, Tomoya
Sagawa, Hiroyuki
Cheoun, Myung-Ki
contents We present a relativistic mean-field model that incorporates charge symmetry breaking (CSB) of nuclear force via $ ω$-$ ρ^0 $ meson mixing, along with corrections to the electromagnetic interaction including the nucleon form factors, first-order vacuum polarization, and Coulomb exchange and pairing terms. The model parameters are refitted using the mass differences of $ T = 1/2 $ mirror nuclei and ground-state properties of magic nuclei, yielding DD-ME-CSB parameter set. The DD-ME-CSB parameter set reproduces the mass differences of mirror nuclei reasonably well up to $ T = 2 $, demonstrating the importance of $ ω$-$ ρ^0 $ mixing. A connection of the present model to a Skyrme-type CSB interaction is also established through a gradient expansion of the energy density functional.
format Preprint
id arxiv_https___arxiv_org_abs_2506_06629
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Charge symmetry breaking effects of $ω$-$ρ^0$ mixing in relativistic mean-field model
Tanimura, Yusuke
Naito, Tomoya
Sagawa, Hiroyuki
Cheoun, Myung-Ki
Nuclear Theory
We present a relativistic mean-field model that incorporates charge symmetry breaking (CSB) of nuclear force via $ ω$-$ ρ^0 $ meson mixing, along with corrections to the electromagnetic interaction including the nucleon form factors, first-order vacuum polarization, and Coulomb exchange and pairing terms. The model parameters are refitted using the mass differences of $ T = 1/2 $ mirror nuclei and ground-state properties of magic nuclei, yielding DD-ME-CSB parameter set. The DD-ME-CSB parameter set reproduces the mass differences of mirror nuclei reasonably well up to $ T = 2 $, demonstrating the importance of $ ω$-$ ρ^0 $ mixing. A connection of the present model to a Skyrme-type CSB interaction is also established through a gradient expansion of the energy density functional.
title Charge symmetry breaking effects of $ω$-$ρ^0$ mixing in relativistic mean-field model
topic Nuclear Theory
url https://arxiv.org/abs/2506.06629