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nucl-th 1

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2026 1

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Astrophysical S-factor Calculation for p-p Fusion Reaction

nucl-th · 2026-07-01 · reject · novelty 5.0

Using a finite-range inverse potential and full WKB tunneling integral instead of the bare Coulomb Gamow factor, the authors obtain S(0) = (1.26±0.04)×10^-26 MeV·b, ~30× below the standard value.

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  • Astrophysical S-factor Calculation for p-p Fusion Reaction nucl-th · 2026-07-01 · reject · none · ref 6

    Using a finite-range inverse potential and full WKB tunneling integral instead of the bare Coulomb Gamow factor, the authors obtain S(0) = (1.26±0.04)×10^-26 MeV·b, ~30× below the standard value.