Thermonuclear processes of the Universe

TL;DR

This book explores nuclear astrophysics processes, modeling light nuclei reactions with potential two-cluster models, calculating astrophysical S-factors, and demonstrating good agreement with experimental data.

Contribution

It introduces a potential two-cluster model for light nuclei and applies it to photonuclear reactions, providing accurate S-factor calculations for astrophysical energies.

Findings

Successful description of experimental data for light nuclei reactions.

Calculation of astrophysical S-factors for multiple nuclear channels.

Validation of the potential two-cluster model in nuclear astrophysics.

Abstract

The book considers some theoretical questions of nuclear astro-physics thermal energies and light atomic nuclei. For the analysis of re-actions is used potential two cluster model of light nuclei with classifica-tion of states by orbital schemes. On its basis photonuclear processes in p2H, p3H, p6Li, p7Li, p9Be and p12C, and also 2H4He, 3H4He, 3He4He and 4He12C channels are considered and astrophysical S - factors corre-sponding to them are calculated. It is shown, that used methods allow to describe well available experimental data in the field of astrophysical energies. This Book is written in Russian, but will perhaps present certain interest.