activity
19992008
most citedAstrophysical S-factor of the 3He(alpha,gamma)7Be reaction measured at low energy via prompt and delayed gamma detection

140 citations · 418 across the 7 of their papers we have counts for

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12 papers · 1 filter

nucl-ex200949 cited

Direct measurement of the 15N(p,gamma)16O total cross section at novae energies

D Bemmerer, A Caciolli, R Bonetti +21

The 15N(p,gamma)16O reaction controls the passage of nucleosynthetic material from the first to the second carbon-nitrogen-oxygen (CNO) cycle. A direct measurement of the total 15N…

nucl-ex200871 cited

Ultra-sensitive in-beam gamma-ray spectroscopy for nuclear astrophysics at LUNA

A. Caciolli, L. Agostino, D. Bemmerer +29

Ultra-sensitive in-beam gamma-ray spectroscopy studies for nuclear astrophysics are performed at the LUNA (Laboratory for Underground Nuclear Astrophysics) 400 kV accelerator, deep…

nucl-ex200883 cited

The 3He(alpha,gamma)7Be S-factor at solar energies: the prompt gamma experiment at LUNA

H. Costantini, D. Bemmerer, F. Confortola +28

The 3He(alpha,gamma)7Be process is a key reaction in both Big-Bang nucleosynthesis and p-p chain of Hydrogen Burning in Stars. A new measurement of the 3He(alpha,gamma)7Be cross se…

nucl-ex200896 cited

Precision study of ground state capture in the 14N(p,gamma)15O reaction

M. Marta, A. Formicola, Gy. Gyurky +28

The rate of the hydrogen-burning carbon-nitrogen-oxygen (CNO) cycle is controlled by the slowest process, 14N(p,gamma)15O, which proceeds by capture to the ground and several excit…

nucl-ex20077 cited

Measurement of 25Mg(p; gamma)26Al resonance strengths via gamma spectrometry

A. Formicola, A. Best, G. Imbriani +28

The COMPTEL instrument performed the first mapping of the 1.809 MeV photons in the Galaxy, triggering considerable interest in determing the sources of interstellar 26Al. The predi…

nucl-ex20072 cited

Ground state capture in N(p,)O studied above the 259 keV resonance at LUNA

H. P. Trautvetter, D. Bemmerer, R. Bonetti +29

We report on a new measurement of N(p,)O for the ground state capture transition at = 360, 380 and 400 keV, using the 400 kV LUNA accelerator. The true coinc…