Showing 1–20 of 20 results
/ Date/ Name
Nov 28, 2012Impact of a revised $^{25}$Mg(p,$γ$)$^{26}$Al reaction rate on the operation of the Mg-Al cycleOct 1, 2012Preparation and characterisation of isotopically enriched Ta$_2$O$_5$ targets for nuclear astrophysics studiesDec 14, 2011The 25Mg(p,g)Al reaction at low astrophysical energiesJul 22, 2011Revision of the 15N(p,γ)16O reaction rate and oxygen abundance in H-burning zonesMar 28, 2011The 14N(p,gamma)15O reaction studied with a composite germanium detectorNov 10, 2010Constraining the S factor of 15N(p,g)16O at Astrophysical EnergiesJun 28, 2010New experimental study of low-energy (p,gamma) resonances in magnesium isotopesMar 31, 2010An actively vetoed Clover gamma-detector for nuclear astrophysics at LUNADec 17, 2008Ultra-sensitive in-beam gamma-ray spectroscopy for nuclear astrophysics at LUNAJul 30, 2008Precision study of ground state capture in the 14N(p,gamma)15O reactionApr 11, 2008Lifetime measurement of the 6792 keV state in 15O, important for the astrophysical S factor extrapolation in 14N(p,g)15OOct 23, 2007Measurement of 25Mg(p; gamma)26Al resonance strengths via gamma spectrometryAug 24, 2007Ground state capture in $^{14}$N(p,$γ$)$^{15}$O studied above the 259 keV resonance at LUNAJul 31, 2007Comparison of the LUNA 3He(alpha,gamma)7Be activation results with earlier measurements and model calculationsMay 15, 2007Astrophysical S-factor of the 3He(alpha,gamma)7Be reaction measured at low energy via prompt and delayed gamma detectionNov 29, 2005First direct measurement of the total cross section of 12C(alpha,gamma)16OSep 1, 2005S-factor of 14N(p,gamma)15O at astrophysical energiesMar 2, 2004The bottleneck of the CNO burning and the age of the Globular ClustersFeb 10, 1999First Measurement of the He3+He3-->He4+2p Cross Section down to the Lower Edge of the Solar Gamow PeakJul 10, 1997The Cross Section of 3He(3He,2p)4He measured at Solar Energies