activity
20092026
most citedImproved Direct Measurement of the 64.5 keV Resonance Strength in the 17O(p,a)14N Reaction at LUNA

76 citations · 1.9k across the 69 of their papers we have counts for

collaborators

70 papers

nucl-ex2026

O(p,)F Reaction and the C and O Isotopic Ratios in Red Giant Branch Stars

D. Robb, P. McGlynn, M. Aliotta +55

The O/O isotopic ratio is a widely used tracer of nucleosynthesis and mixing processes in red giant stars. Its value depends on the rates of the proton-capture reacti…

nucl-ex2026

The 3He(α,γ)7Be γ-ray angular distribution: measured, and calculated by effective field theory

S. Turkat, P. Hempel, X. Zhang +26

The 3He(alpha,gamma)7Be reaction takes place in several distinct astrophysical scenarios. First, in solar hydrogen burning, 3He(alpha,gamma)7Be controls the competition between the…

physics.ins-det2026

Detector characterization for a new C+C reaction study at LUNA

R. M. Gesùè, S. Turkat, J. Skowroński +50

The C+C fusion reaction plays a crucial role in stellar evolution, including the occurrence of supernova explosions, and in the synthesis of the chemical elements. Ho…

nucl-ex2025

Nonresonant capture cross section measurement of the 29Si(p,gamma)30P reaction

Zs Mátyus, L Csedreki, Zs Fülöp +5

The isotopic ratios measured in meteoritic presolar grains are a crucial tool for tracing the nucleosynthetic origin of isotopes. In the case of silicon isotopes, two important ind…

physics.ins-det2025

Solid Target production for Astrophysical Reasearch: the European target laboratory partnership in ChETEC-INFRA

Roberta Spartà, Alexandra Spiridon, Rosanna Depalo +28

The joint work of European target laboratories in the ChETEC-INFRA project is presented, to face the new experimental challenges of nuclear astrophysics. In particular, results are…

physics.ins-det2025★ 2 cited

Measurement of -particles to determine cross sections relevant to the weak r-process

Sándor R. Kovács, Tibor Norbert Szegedi, Ákos Tóth +9

The neutron-rich isotopes with 30 Z 45 are thought to be synthesised in neutrino-driven winds after the collapse of a massive star. This nucleosynthesis scenario, cal…