English

Revisiting proton-proton fusion in chiral effective field theory

Nuclear Theory 2023-07-26 v2 Solar and Stellar Astrophysics High Energy Physics - Phenomenology

Abstract

We calculate the SS-factor for proton-proton fusion using chiral effective field theory interactions and currents. By performing order-by-order calculations with a variety of chiral interactions that are regularized and calibrated in different ways, we assess the uncertainty in the SS-factor from the truncation of the effective field theory expansion and from the sensitivity of the SS-factor to the short-distance axial current determined from three- and four-nucleon observables. We find that S(0)=(4.100±0.019(syst)±0.013(stat)±0.008(gA))×1023 MeVfm2,S(0)=(4.100\pm0.019\mathrm{(syst)}\pm0.013\mathrm{(stat)}\pm0.008(g_A))\times10^{-23}~\mathrm{MeV\,fm}^2\,, where the three uncertainties arise, respectively, from the truncation of the effective field theory expansion, use of the two-nucleon axial current fit to few-nucleon observables and variation of the axial coupling constant within the recommended range. The increased value of S(0)S(0) compared to previous calculations is mainly driven by an increase in the recommended value for the axial coupling constant and is in agreement with a recent analysis based on pionless effective field theory.

Keywords

Cite

@article{arxiv.2304.03327,
  title  = {Revisiting proton-proton fusion in chiral effective field theory},
  author = {Bijaya Acharya and Laura Elisa Marcucci and Lucas Platter},
  journal= {arXiv preprint arXiv:2304.03327},
  year   = {2023}
}