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Constraining the astrophysical origin of the p-nuclei through nuclear physics and meteoritic data
TLDR
The main part of the review focuses on the nuclear uncertainties involved in the determination of the astrophysical reaction rates required for the extended reaction networks used in nucleosynthesis studies.
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The baryon density of the Universe from an improved rate of deuterium burning.
TLDR
Improved cross-sections of the deuterium burning D(p,γ)3He reaction lead to BBN estimates of the baryon density at the 1.6 percent level, in excellent agreement with a recent analysis of the cosmic microwave background.
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S-factor of 14N(p,γ)15O at astrophysical energies⋆
Abstract.The astrophysical S(E) factor of 14N(p,γ)15O has been measured for effective center-of-mass energies between Eeff = 119 and 367 keV at the LUNA facility using TiN solid targets and Ge…
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Improved Direct Measurement of the 64.5 keV Resonance Strength in the ^{17}O(p,α)^{14}N Reaction at LUNA.
TLDR
A new direct determination of the E_{R}=64.5  keV resonance strength performed at the Laboratory for Underground Nuclear Astrophysics (LUNA) accelerator has led to the most accurate value to date ωγ=10.0±1.4_{stat}±0.7_{syst}‬neV, thanks to a significant background reduction underground and generally improved experimental conditions.
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Half-life of 44Ti
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Experimental study of proton-induced nuclear reactions in 6,7 Li
The 6Li(p,α)3He and 7Li(p,α)4He reaction cross sections were obtained for E = 90–580 keV and E = 90–1740 keV, respectively. R-matrix and polynomial fits to the bare astrophysical S-factor confirmed,…
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First measurement of the d(p,γ)3He cross section down to the solar Gamow peak
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N=14 and 16 shell gaps in neutron-rich oxygen isotopes
In-beam gamma-ray spectroscopy using fragmentation reactions of both stable and radioactive beams has been performed in order to study the structure of excited states in neutron-rich oxygen isotopes…
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Electron screening effect in the reactions 3He(d, p) 4He and d( 3He, p) 4He ? ? Supported in part by
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Electron screening in 7Li(p,α)α and 6Li(p,α)3He for different environments
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