77 citations · 166 across the 6 of their papers we have counts for
6 papers
Towards a comprehensive study of the 14N(p,g)15O astrophysical key reaction: Description of the experimental technique including novel target preparation
A. Compagnucci, A. Formicola, M. Campostrini +46
While the 14N(p,g)15O reaction plays a key role in the hydrogen-burning processes in various stellar conditions, its reaction rate is not known with sufficient precision. Therefore…
Characterization of the LUNA neutron detector array for the measurement of the 13C(a,n)16O reaction
L. Csedreki, G. F. Ciani, J. Balibrea-Correa +46
We introduce the LUNA neutron detector array developed for the investigation of the 13C(a,n)16O reaction towards its astrophysical s-process Gamow peak in the low-background enviro…
First direct limit on the 334 keV resonance strength in the Ne(α,γ)Mg reaction
D. Piatti, E. Masha, M. Aliotta +44
In stars, the fusion of Ne and He may produce either Mg, with the emission of a neutron, or Mg and a ray. At high temperature, the () channel domi…
Test of statistical model cross section calculations for -induced reactions on Ag at energies of astrophysical interest
C. Yalcin, Gy. Gyürky, T. Rauscher +8
Astrophysical reaction rates, which are mostly derived from theoretical cross sections, are necessary input to nuclear reaction network simulations for studying the origin of n…
The 25Mg(p,g)Al reaction at low astrophysical energies
LUNA Collaboration, F. Strieder, B. Limata +28
In the present work we report on a new measurement of resonance strengths in the reaction 25Mg(p,gamma)26Al at E_cm= 92 and 189 keV. This study was performed at the LUNA facility i…
Absolute measurement of the 5/2+ resonance of 36Ar(p,gamma)37K at E_p = 918 keV
P. Mohr, H. Oberhummer, Gy. Gyürky +3
The strength of the 5/2+ resonance of the reaction 36Ar(p,gamma)37K at E_p = 918 keV was measured absolutely: omega gamma = (258 \pm 24) meV. The new result is consistent with prev…