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- W1978926437 abstract "The proton burning process p + p -> d + e(+) + nu(e), important for the stellar evolution of main-sequence stars of mass equal to or less than that of the Sun, is computed in effective field theory using chiral perturbation expansion to the next-to-next-to leading chiral order. This represents a model-independent calculation consistent with low-energy effective theory of QCD comparable in accuracy to the radiative np capture at thermal energy previously calculated by first using very accurate two-nucleon wavefunctions backed up by an effective field theory technique with a finite cut-off. The result obtained thereby is found to support within theoretical uncertainties the previous calculation of the same process by Bahcall and his co-workers." @default.
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- W1978926437 date "1998-11-01" @default.
- W1978926437 modified "2023-09-30" @default.
- W1978926437 title "The Solar Proton Burning Process Revisited in Chiral Perturbation Theory" @default.
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- W1978926437 doi "https://doi.org/10.1086/306331" @default.
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