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C. Bruno

29 papers hereh-index 19961 citations83 works total

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

author position
  • first author1
  • middle author21

Across the 22 of 29 papers where every author was matched, so the position is known.

fields
  • nucl-ex22
  • physics.ins-det4
  • astro-ph.SR3
same name
  • C. Bruno — 4 papers, h 3
  • C. Bruno — 1 paper, h 10
  • C. Bruno — 1 paper, h 3

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

activity
20142026
most citedImproved Direct Measurement of the 64.5 keV Resonance Strength in the 17O(p,a)14N Reaction at LUNA

76 citations · 674 across the 28 of their papers we have counts for

collaborators
Showing 2016 · nucl-exShow all

3 papers · 2 filters

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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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.