# The limits of the nuclear landscape explored by the relativistic   continuum Hatree-Bogoliubov theory

**Authors:** X. W. Xia, Y. Lim, P. W. Zhao, H. Z. Liang, X. Y. Qu, Y. Chen, H. Liu,, L. F. Zhang, S. Q. Zhang, Y. Kim, J. Meng

arXiv: 1704.08906 · 2018-06-05

## TL;DR

This paper uses the relativistic continuum Hartree-Bogoliubov theory to extensively predict the properties and boundaries of nuclei across a wide range of atomic numbers, significantly extending the known nuclear landscape.

## Contribution

It introduces a comprehensive RCHB-based approach that includes continuum effects and pairing correlations, providing new predictions for nuclear stability and properties.

## Key findings

- 9035 nuclei predicted to be bound, extending the nuclear landscape.
- Continuum coupling and pairing correlations are crucial for landscape extension.
- Predictions include binding energies, radii, and decay energies.

## Abstract

The ground-state properties of nuclei with 8 $\le$ Z $\le$ 120 from the proton drip line to the neutron drip line have been investigated using the relativistic continuum Hartree-Bogoliubov (RCHB) theory with the relativistic density functional PC-PK1. With the effects of the continuum included, there are totally 9035 nuclei predicted to be bound, which largely extends the existing nuclear landscapes predicted with other methods. The calculated binding energies, separation energies, neutron and proton Fermi surfaces, root-mean-square (rms) radii of neutron, proton, matter, and charge distributions, ground-state spins and parities are tabulated. The extension of the nuclear landscape obtained with RCHB is discussed in detail, in particular for the neutron-rich side, in comparison with the relativistic mean field calculations without pairing correlations and also other predicted landscapes. It is found that the coupling between the bound states and the continuum due to the pairing correlations plays an essential role in extending the nuclear landscape. The systematics of the separation energies, radii, densities, potentials and pairing energies of the RCHB calculations are also discussed. In addition, the alpha-decay energies and proton emitters based on the RCHB calculations are investigated.

## Figures

35 figures with captions in the complete paper: https://tomesphere.com/paper/1704.08906/full.md

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Source: https://tomesphere.com/paper/1704.08906