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Helioseismology and p+p $\to$ d + e$^+$ + $\nu _e$ in the sun

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arxiv astro-ph/9707133 v1 pith:25LNEAUP submitted 1997-07-11 astro-ph

classification astro-ph
keywords modelhelioseismichelioseismologysolaraccordingadoptedapproachcalculations
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abstract

By using a phenomenological field theory of nucleon-nucleon interactions, Oberhummer et al. found a cross section of p+p $\to$ d + e$^+$ + $\nu _e$ about 2.9 times that given by the potential approach and adopted in Standard Solar Model calculations. We show that a solar model with $S=2.9 S_{SSM}$ is inconsistent with helioseismic data, the difference between model predictions and helioseismic determinations being typically a factor ten larger than estimated uncertainties. We also show that, according to helioseismology, $\Sppzero$ cannot differ from $S_{SSM}$ by more than 15%.

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