Statistical Spectroscopy for Neutron-rich sd-Shell Nuclei

TL;DR

This paper applies spectral distribution theory to analyze neutron-rich sd-shell nuclei, providing statistical spectroscopic results that align with experimental data and are useful for nuclear astrophysics applications.

Contribution

It introduces the use of spectral distribution theory for neutron-rich sd-shell nuclei, offering a new statistical approach to nuclear structure analysis.

Findings

Spectroscopic results agree with experimental data.

Provides averaged nuclear properties relevant for astrophysics.

Demonstrates the applicability of spectral distribution theory to neutron-rich nuclei.

Abstract

Statistical spectroscopic results using the spectral distribution theory are obtained for the structure of neutron-rich light nuclei going towards the drip line and compared to experimental values available. These results will be useful for nuclear astrophysics problems where often averaged nuclear properties are adequate.