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A. Di Leva

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

fields
  • nucl-ex3
  • astro-ph.SR1
ORCID 0000-0002-8762-0522
same name
  • A. Di Leva — 2 papers, h 10

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

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

76 citations · 197 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2016★ 49 cited

22Ne and 23Na ejecta from intermediate-mass stars: The impact of the new LUNA rate for 22Ne(p,γ)23Na

A. Slemer, P. Marigo, D. Piatti +36

We investigate the impact of the new LUNA rate for the nuclear reaction 22Ne(p,γ)23Na on the chemical ejecta of intermediate-mass stars, with particular focus on the ther…

nucl-ex2016★ 17 cited

Shell and explosive hydrogen burning

A. Boeltzig, C. G. Bruno, F. Cavanna +10

The nucleosynthesis of light elements, from helium up to silicon, mainly occurs in Red Giant and Asymptotic Giant Branch stars and Novae. The relative abundances of the synthesized…

nucl-ex2016★ 55 cited

Direct measurement of low-energy 22Ne(p,γ)23Na resonances

R. Depalo, F. Cavanna, M. Aliotta +30

The 22Ne(p,γ)23Na reaction is the most uncertain process in the neon-sodium cycle of hydrogen burning. At temperatures relevant for nucleosynthesis in asymptotic giant…

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 17O(p,α)14N reaction plays a key role in various astrophysical scenarios, from asymptotic giant branch stars to classical novae. It affects the synthesis of rare is…

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