1999
DOI: 10.1016/s0375-9474(99)00314-0
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Proton-proton fusion in leading order of effective field theory

Abstract: Using a recently developed effective field theory for the interactions of nucleons at non-relativistic energies, we calculate the rate for the fusion process p + p → d + e + + ν e to leading order in the momentum expansion. Coulomb effects are included non-perturbatively in a systematic way. The resulting rate is independent of specific models for the strong interactions at short distances and is in agreement with the standard result in the zero-range approximation.The first step in the different nuclear proce… Show more

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Cited by 63 publications
(93 citation statements)
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“…This is a good approximation because the difference between the amplitude from the effective range theory, which is almost the same as our LO result, and that from accurate potential model calculations Our result KR(NLO) [16] Table 1: Estimated values of Λ 2 (0). The value in second column is our result.…”
Section: Numerical Resultssupporting
confidence: 67%
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“…This is a good approximation because the difference between the amplitude from the effective range theory, which is almost the same as our LO result, and that from accurate potential model calculations Our result KR(NLO) [16] Table 1: Estimated values of Λ 2 (0). The value in second column is our result.…”
Section: Numerical Resultssupporting
confidence: 67%
“…The value in second column is our result. The values in third, fourth, and fifth column are estimated from the pionless EFT calculation up to NLO by Kong and Ravndal (KR) [16], that up to N 4 LO by Butler and Chen (BC) [17], and an accurate phenomenological potential model calculation [11], respectively.…”
Section: Numerical Resultsmentioning
confidence: 99%
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“…The relative size of the contribution of an operator to a particular observable can be estimated by the power-counting rules developed in [1][2][3][4][5][6][7]. An array of phenomena have been studied with EFT(π /), such as the radiative capture np → dγ relevant to Big-Bang nucleosynthesis [9,10], elastic and inelastic νd scattering [11,12] relevant to the ongoing efforts to measure the solar-neutrino flux and the cross section for pp → deν [13][14][15][16], the electromagnetic form factors of the deuteron [7,17], and other processes involving electroweak gauge fields (for a detailed review of this subject see Ref. [18]).…”
Section: Introductionmentioning
confidence: 99%
“…In the Standard Solar Model (SSM) [28] the total (or bolometric) luminosity of the Sun L ⊙ = (3.846 ± 0.008) × 10 26 W is normalized to the astrophysical factor S pp (0) for the solar proton burning. The recommended value S pp (0) = 4.00×10 −25 MeVb [29] has been found by averaging over the results obtained in the Potential model approach (PMA) [30,31] and the Effective Field Theory (EFT) approach [32,33]. As has been shown recently in Ref.…”
Section: Introductionmentioning
confidence: 99%