activity
20122018
most citedImproved Direct Measurement of the 64.5 keV Resonance Strength in the 17O(p,a)14N Reaction at LUNA

76 citations · 250 across the 6 of their papers we have counts for

collaborators

6 papers

nucl-ex2018★ 16 cited

Effect of beam energy straggling on resonant yield in thin gas targets: The cases Ne(p,γ)Na and N(p,γ)O

D. Bemmerer, F. Cavanna, R. Depalo +25

When deriving resonance strengths using the thick-target yield approximation, for very narrow resonances it may be necessary to take beam energy straggling into account. This appli…

astro-ph.SR2017

Origin of meteoritic stardust unveiled by a revised proton-capture rate of O

M. Lugaro, A. I. Karakas, C. G. Bruno +34

Stardust grains recovered from meteorites provide high-precision snapshots of the isotopic composition of the stellar environment in which they formed. Attributing their origin to…

nucl-ex2016★ 76 cited

Improved Direct Measurement of the 64.5 keV Resonance Strength in the 17O(p,a)14N Reaction at LUNA

C. G. Bruno, D. A. Scott, M. Aliotta +32

The O(p,)N reaction plays a key role in various astrophysical scenarios, from asymptotic giant branch stars to classical novae. It affects the synthesis of rare is…

nucl-ex2015★ 71 cited

Three new low-energy resonances in the Ne(p,)Na reaction

F. Cavanna, R. Depalo, M. Aliotta +31

The Ne(p,)Na reaction takes part in the neon-sodium cycle of hydrogen burning. This cycle affects the synthesis of the elements between Ne and Al in…

nucl-ex2013★ 34 cited

Neutron-induced background by an alpha-beam incident on a deuterium gas target and its implications for the study of the 2H(alpha,gamma)6Li reaction at LUNA

M. Anders, D. Trezzi, A. Bellini +26

The production of the stable isotope Li-6 in standard Big Bang nucleosynthesis has recently attracted much interest. Recent observations in metal-poor stars suggest that a cosmolog…

nucl-ex2012★ 53 cited

Preparation and characterisation of isotopically enriched TaO targets for nuclear astrophysics studies

A. Caciolli, D. A. Scott, A. Di Leva +33

The direct measurement of reaction cross sections at astrophysical energies often requires the use of solid targets of known thickness, isotopic composition, and stoichiometry that…