The radiative 10Be(n,g)11be capture at thermal and astrophysical energies

TL;DR

This paper models the neutron radiative capture on 10Be at thermal and astrophysical energies using a modified potential cluster approach, successfully describing experimental cross section data.

Contribution

It introduces a modified potential cluster model with forbidden states and Young tableaux classification to accurately predict reaction cross sections.

Findings

Model reproduces experimental cross sections

Validates the modified potential cluster approach

Applicable to astrophysical energy ranges

Abstract

Within the framework of the modified potential cluster model with the forbidden states and the classification of states according to Young tableaux the possibility of describing the available experimental data for the total reaction cross sections of the neutron radiative capture on 10Be at thermal and astrophysical energies was shown.