2006
DOI: 10.1016/j.nuclphysa.2004.09.008
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Modern theories of low-energy astrophysical reactions

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Cited by 49 publications
(51 citation statements)
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References 121 publications
(205 reference statements)
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“…The observed abundances of D, 3 He, and 4 He are in good agreement with calculations, confirming the overall validity of BBN theory. On the other hand, the observed abundance of 7 Li is a factor 2 ÷ 3 lower than the predicted abundance (see Fig.…”
Section: Introductionsupporting
confidence: 80%
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“…The observed abundances of D, 3 He, and 4 He are in good agreement with calculations, confirming the overall validity of BBN theory. On the other hand, the observed abundance of 7 Li is a factor 2 ÷ 3 lower than the predicted abundance (see Fig.…”
Section: Introductionsupporting
confidence: 80%
“…Everything is enclosed in a radon box flushed with high purity N 2 , to reduce and stabilize the γ activity due to the radon decay chain. 3 He reaction (E n(cm) = 2450 keV) induce (n,n γ) reactions in the Ge detector and in the surrounding materials (lead, steel, copper), generating a beam-induced background in the γ-ray spectrum, in particular around 1.6 MeV, where the capture transition to the ground state of 6 Li is expected. To reduce the neutron production, a tube 16 cm long, with a square cross section of 2 × 2 cm 2 is inserted inside the chamber.…”
Section: Experimental Set-upmentioning
confidence: 99%
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“…The AV18/UIX Hamiltonian quantitatively and successfully accounts for a wide variety of few-nucleon bound-state properties and reactions, ranging from binding energies and charge radii to electromagnetic form factors, low-energy scattering observables and electroweak capture cross sections (for a review, see Refs. [11,12]). …”
Section: Introductionmentioning
confidence: 99%