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arXiv:nucl-th/0107012·v2·Nuclear Theory

The Solar hep Process in Effective Field Theory

T.-S. Park🇺🇸 · L.E. Marcucci🇮🇹 · R. Schiavilla🇺🇸 · M. Viviani🇮🇹 · A. Kievsky🇮🇹 · S. Rosati🇮🇹 · K. Kubodera🇺🇸 · D.-P. Min🇰🇷 · M. Rho🇰🇷

Abstract

Using effective field theory, we calculate the S-factor for the hep process in a totally parameter-free formulation. The transition operators are organized according to chiral counting, and their matrix elements are evaluated using the realistic nuclear wave functions obtained in the correlated-hyperspherical-harmonics method. Terms of up to next-to-next-to-next-to-leading order in heavy-baryon chiral perturbation theory are considered. Fixing the only parameter in the theory by fitting the tritium \beta-decay rate, we predict the hep S-factor with accuracy better than \sim 20 %.

Comments: 4 pages, Revtex. Minor revision has been made

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