The Nucleosynthesis and Reaction Rates of Fluorine 19 ($^{19}F$) in the Sun. (arXiv:1904.09608v1 [astro-ph.SR])

The Nucleosynthesis and Reaction Rates of Fluorine 19 ($^{19}F$) in the Sun. (arXiv:1904.09608v1 [astro-ph.SR])
<a href="http://arxiv.org/find/astro-ph/1/au:+Mardini_M/0/1/0/all/0/1">Mohammad K. Mardini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ershiadat_N/0/1/0/all/0/1">Nidal Ershiadat</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Al_Wardat_M/0/1/0/all/0/1">Mashhoor A. Al-Wardat</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Taani_A/0/1/0/all/0/1">Ali A. Taani</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ozdemir_S/0/1/0/all/0/1">Sergen Ozdemir</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Al_Naimiy_H/0/1/0/all/0/1">Hamid Al-Naimiy</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Khasawneh_A/0/1/0/all/0/1">Awni Khasawneh</a>

We investigate the abundance of $^{19}F$ in the Sun through the
nucleosynthesis scenario. In addition, we calculate the rate equations and
reaction rates of the nucleosynthesis of $^{19}F$ at different temperature
scale. Other important functions of this nucleosynthesis (nuclear partition
function and statistical equilibrium conditions) are also obtained. The
resulting 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 and
beta-decay until $^{19}F$ is produced. The reaction rate of $^{15}N$ ($alpha$,
$gamma$) $^{19}F$ was dominated by the contribution of three low-energy
resonances, which enhanced the final $^{19}F$ abundance in the envelope.

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