Showing 1–20 of 26 results
/ Date/ Name
May 16, 2022Horizons: Nuclear Astrophysics in the 2020s and BeyondMar 1, 2017Origin of meteoritic stardust unveiled by a revised proton-capture rate of $^{17}$ONov 2, 2016The impact of the revised $^{17}$O$(p,α)^{14}$N reaction rate on $^{17}$O stellar abundances and yieldsOct 3, 2016Improved Direct Measurement of the 64.5 keV Resonance Strength in the 17O(p,a)14N Reaction at LUNAOct 6, 2013Nuclear astrophysics with radioactive ions at FAIRNov 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 detection