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Improved astrophysical rate for the 18O(p,α)15N reaction by underground measurements
Free accessDOAJ | 2019| -
Direct measurements of low-energy resonance strengths of the 23Na(p,γ)24Mg reaction for astrophysics
Free accessDOAJ | 2019| -
β-delayed neutron emission of r-process nuclei at the N = 82 shell closure
Free accessDOAJ | 2021| -
A new study of the 22Ne(p,gamma)23Na reaction deep underground: Feasibility, setup and first observation of the 186 keV resonance
Free accessBASE | 2014|Contributors: C.G. Bruno -
22Ne and 23Na ejecta from intermediate-mass stars: the impact of the new LUNA rate for 22Ne(p,γ)23Na
Free accessBASE | 2017|Contributors: C.G. Bruno -
The impact of the revised 17O(p; alpha)14N reaction rate on 17O stellar abundances and yields
Free accessBASE | 2017|Contributors: C.G. Bruno -
The baryon density of the Universe from an improved rate of deuterium burning
Free accessBASE | 2020|Contributors: C.G. Bruno -
Cross section of the reaction 18O(p,γ)19F at astrophysical energies: The 90 keV resonance and the direct capture component
Free accessBASE | 2019|Contributors: C.G. Bruno -
First direct limit on the 334 keV resonance strength in $$^{22}$$Ne($$\alpha $$,$$\gamma $$)$$^{26}$$Mg reaction [First direct limit on the 334 keV resonance strength in Ne-22(alpha, gamma)Mg-26 reaction]
Free accessBASE | 2022|Contributors: C.G. Bruno
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