Charge symmetry breaking in hypernuclei within RMF model

Fuente: arXiv
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Auteurs principaux: Sun, Ting-Ting, Tanimura, Yusuke, Sagawa, Hiroyuki, Hiyama, Emiko
Format: Preprint
Publié: 2025
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author Sun, Ting-Ting
Tanimura, Yusuke
Sagawa, Hiroyuki
Hiyama, Emiko
author_facet Sun, Ting-Ting
Tanimura, Yusuke
Sagawa, Hiroyuki
Hiyama, Emiko
contents We study the charge symmetry breaking (CSB) effect in the binding energy of mirror hypernuclei in the mass region $A=7\sim 48$ in relativistic mean field (RMF) models introducing $NN$ and $ΛN$ interactions. The phenomenological $ΛN$ CSB interaction is introduced and the strength parameter is fitted to reproduce the experimental binding energy difference between the mirror hypernuclei $^{12}_Λ$B and $^{12}_Λ$C. This model is applied to calculate the CSB energy anomaly in mirror hypernuclei with the mass $A=7\sim48$. The model is further applied to predict the binding energy difference of mirror hypernuclei of $A$=40 with the isospin $T=1/2$, $3/2$ and $5/2$ nuclei together with various hyper Ca isotopes and their mirror hypernuclei. Finally the binding energy systematics of $A=$48 hypernuclei are predicted with/without the CSB effect by the PK1 and TM2 energy density functionals (EDFs).
format Preprint
id arxiv_https___arxiv_org_abs_2502_21161
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Charge symmetry breaking in hypernuclei within RMF model
Sun, Ting-Ting
Tanimura, Yusuke
Sagawa, Hiroyuki
Hiyama, Emiko
Nuclear Theory
We study the charge symmetry breaking (CSB) effect in the binding energy of mirror hypernuclei in the mass region $A=7\sim 48$ in relativistic mean field (RMF) models introducing $NN$ and $ΛN$ interactions. The phenomenological $ΛN$ CSB interaction is introduced and the strength parameter is fitted to reproduce the experimental binding energy difference between the mirror hypernuclei $^{12}_Λ$B and $^{12}_Λ$C. This model is applied to calculate the CSB energy anomaly in mirror hypernuclei with the mass $A=7\sim48$. The model is further applied to predict the binding energy difference of mirror hypernuclei of $A$=40 with the isospin $T=1/2$, $3/2$ and $5/2$ nuclei together with various hyper Ca isotopes and their mirror hypernuclei. Finally the binding energy systematics of $A=$48 hypernuclei are predicted with/without the CSB effect by the PK1 and TM2 energy density functionals (EDFs).
title Charge symmetry breaking in hypernuclei within RMF model
topic Nuclear Theory
url https://arxiv.org/abs/2502.21161