English

Ab Initio Description of p-Shell Hypernuclei

Nuclear Theory 2014-11-05 v2 Solar and Stellar Astrophysics High Energy Physics - Phenomenology

Abstract

We present the first ab initio calculations for p-shell single-Lambda hypernuclei. For the solution of the many-baryon problem, we develop two variants of the no-core shell model with explicit Λ\Lambda and Σ+\Sigma^+, Σ0\Sigma^0, Σ\Sigma^- hyperons including Λ\Lambda-Σ\Sigma conversion, optionally supplemented by a similarity renormalization group transformation to accelerate model-space convergence. In addition to state-of-the-art chiral two- and three-nucleon interactions, we use leading-order chiral hyperon-nucleon interactions and a recent meson-exchange hyperon-nucleon interaction. We validate the approach for s-shell hypernuclei and apply it to p-shell hypernuclei, in particular to Λ7^7_\LambdaLi, Λ9^9_\LambdaBe and Λ13^{13}_\LambdaC. We show that the chiral hyperon-nucleon interactions provide ground-state and excitation energies that agree with experiment within the cutoff dependence. At the same time we demonstrate that hypernuclear spectroscopy provides tight constraints on the hyperon-nucleon interactions and we discuss the impact of induced hyperon-nucleon-nucleon interactions.

Keywords

Cite

@article{arxiv.1403.3067,
  title  = {Ab Initio Description of p-Shell Hypernuclei},
  author = {Roland Wirth and Daniel Gazda and Petr Navrátil and Angelo Calci and Joachim Langhammer and Robert Roth},
  journal= {arXiv preprint arXiv:1403.3067},
  year   = {2014}
}

Comments

6 pages, 4 figures

R2 v1 2026-06-22T03:25:28.876Z