English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We investigate the abundance of $^{19}F$ in the Sun through thenucleosynthesis scenario. In addition, we calculate the rate equations andreaction rates of the nucleosynthesis of $^{19}F$ at different temperaturescale. Other important functions of this nucleosynthesis (nuclear partitionfunction and statistical equilibrium conditions) are also obtained. Theresulting stability of $^{19}F$ occurs at nucleus with A = 19 and Mass Excess=-1.4874 MeV. As a result, this will tend to a series of neutron captures andbeta-decay until $^{19}F$ is produced. The reaction rate of $^{15}N$ ($\alpha$,$\gamma$) $^{19}F$ was dominated by the contribution of three low-energyresonances, which enhanced the final $^{19}F$ abundance in the envelope.

The Nucleosynthesis and Reaction Rates of Fluorine 19 ($^{19}F$) in the Sun