By using a phenomenological field theory of nucleon-nucleon interactions, Oberhummer et al. found a cross section of p + p → d + e+ + νe 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 = 2.9SSSM 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, S cannot differ from SSSM by more than 15%. © 1998 Elsevier Science B.V.
Helioseismology and p+p $to$ d + e$^+$ + $nu _e$ in the sun
Fiorentini G.;Ricci B.
1998
Abstract
By using a phenomenological field theory of nucleon-nucleon interactions, Oberhummer et al. found a cross section of p + p → d + e+ + νe 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 = 2.9SSSM 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, S cannot differ from SSSM by more than 15%. © 1998 Elsevier Science B.V.File in questo prodotto:
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