He3(α,γ)Be7 and H3(α,γ)Li7 astrophysical S factors from the no-core shell model with continuum-Reference-Cited by-同舟云学术

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He3(α,γ)Be7 and H3(α,γ)Li7 astrophysical S factors from the no-core shell model with continuum

Published:2016-06 Issue: Volume:757 Page:430-436
ISSN:0370-2693
Container-title:Physics Letters B
language:en
Short-container-title:Physics Letters B

Author:

Dohet-Eraly Jérémy,Navrátil Petr,Quaglioni Sofia,Horiuchi Wataru,Hupin Guillaume,Raimondi Francesco

Funder

National Research Council Canada

NSERC

LLNL

U.S. Department of Energy, Office of Science, Office of Nuclear Physics

JSPS

ORNL

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference66 articles.

1. Sharpening the Predictions of Big-Bang Nucleosynthesis

2. Estimating reaction rates and uncertainties for primordial nucleosynthesis

3. Solar fusion cross sections

4. Solar fusion cross sections. II. Theppchain and CNO cycles

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