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A Study of the Abundance of Low-Z Elements in the Sun During its Whole Predicted Life

A Study of the Abundance of Low-Z Elements in the Sun During its Whole Predicted Life The study of the chemical composition of stars and galaxies is a key topic for understanding their origin and evolution. In this study, we present the results of the calculation of solar abundances of the isotopes 1H, 4He, 12C, 14N, 15O, 16O, 17O, and 18O during the four phases of the solar life: hydrogen burning, onset of rapid growth and red giant, helium burning and helium exhaustion. The open source package “NucNet Tools” from the Webnucleo Group in Clemson University, SC, USA was used for this purpose. The results for all isotopes are listed in tables for future use. Abundances found, globally, agree fairly well with those predicted in the literature. Results obtained for the last two phases have no equivalents elsewhere. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Astrophysical Bulletin Springer Journals

A Study of the Abundance of Low-Z Elements in the Sun During its Whole Predicted Life

Talafha, M.; Al-Wardat, M.; Ershaidat, N.
Astrophysical Bulletin , Volume 73 (2) – May 29, 2018
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References (2)

Publisher
Springer Journals
Copyright
Copyright © 2018 by Pleiades Publishing, Ltd.
Subject
Physics; Astronomy, Astrophysics and Cosmology
ISSN
1990-3413
eISSN
1990-3421
DOI
10.1134/S1990341318020098
Publisher site
See Article on Publisher Site

Abstract

The study of the chemical composition of stars and galaxies is a key topic for understanding their origin and evolution. In this study, we present the results of the calculation of solar abundances of the isotopes 1H, 4He, 12C, 14N, 15O, 16O, 17O, and 18O during the four phases of the solar life: hydrogen burning, onset of rapid growth and red giant, helium burning and helium exhaustion. The open source package “NucNet Tools” from the Webnucleo Group in Clemson University, SC, USA was used for this purpose. The results for all isotopes are listed in tables for future use. Abundances found, globally, agree fairly well with those predicted in the literature. Results obtained for the last two phases have no equivalents elsewhere.

Journal

Astrophysical Bulletin – Springer Journals

Published: May 29, 2018

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