English

Molecular-orbital structure in neutron-rich C isotopes

Nuclear Theory 2009-11-07 v1

Abstract

The molecule-like structure of the C isotopes (A=12, 14, 16) is investigated using a microscopic α+α+α+n+n+\alpha+\alpha+\alpha+n+n+\cdot \cdot \cdot model. The valence neutrons are classified based on the molecular-orbit (MO) model, and both π\pi-orbit and σ\sigma-orbit are introduced around three α\alpha-clusters. The valence neutrons which occupy the π\pi-orbit increase the binding energy and stabilize the linear-chain of 3α\alpha against the breathing-like break-up. However, 14^{14}C with the π\pi-orbit does not show clear energy minimum against the bending-like path. The combination of the valence neutrons in the π\pi- and the σ\sigma-orbit is promising to stabilize the linear-chain state against the breathing- and bending- modes, and it is found that the excited states of 16^{16}C with the (3/2π)2(1/2σ)2(3/2^-_\pi)^2(1/2^-_\sigma)^2 configuration for the four valence neutrons is one of the most promising candidates for such structure.

Keywords

Cite

@article{arxiv.nucl-th/0103047,
  title  = {Molecular-orbital structure in neutron-rich C isotopes},
  author = {N. Itagaki and S. Okabe and I. Ikeda and I. Tanihata},
  journal= {arXiv preprint arXiv:nucl-th/0103047},
  year   = {2009}
}

Comments

9 pages, latex, 4 figures