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The European Physical Journal A, ISSN 1434-6001, 3/2018, Volume 54, Issue 3, pp. 1 - 11
The experimental study of nuclear reactions of astrophysical interest is greatly facilitated by a low-background, high-luminosity setup. The Laboratory for... 
Nuclear Physics, Heavy Ions, Hadrons | Nuclear Fusion | Physics | Particle and Nuclear Physics
Journal Article
Physics Letters B, ISSN 0370-2693, 01/2012, Volume 707, Issue 1, pp. 60 - 65
In the present work we report on a new measurement of resonance strengths in the reaction Mg(p,  ) Al at and 189 keV. This study was performed at the LUNA... 
Nuclear astrophysics | Reaction rate | Mg-Al cycle | Proton-capture reaction
Journal Article
PHYSICAL REVIEW LETTERS, ISSN 0031-9007, 10/2018, Volume 121, Issue 17
The Ne-22(p,gamma)Na-23 reaction, part of the neon-sodium cycle of hydrogen burning, may explain the observed anticorrelation between sodium and oxygen... 
NA-23 | CODE | MODELS | PHYSICS, MULTIDISCIPLINARY | THERMONUCLEAR REACTION-RATES | STARS | PATTERNS | NUCLEAR-PHYSICS | NE-22 | GLOBULAR-CLUSTERS
Journal Article
Physical Review Letters, ISSN 0031-9007, 12/2015, Volume 115, Issue 25
The Ne-22(p,gamma)Na-23 reaction takes part in the neon-sodium cycle of hydrogen burning. This cycle affects the synthesis of the elements between Ne-20 and... 
MASSIVE STARS | ELEMENTS | REACTION-RATES | PHYSICS, MULTIDISCIPLINARY | CLASSICAL NOVAE | POPULATIONS | NUCLEOSYNTHESIS | NUCLEAR ASTROPHYSICS | GIANT STARS | CAPTURE | ABUNDANCE
Journal Article
Physical Review C, ISSN 2469-9985, 11/2016, Volume 94, Issue 5
Background: The Ne-22(p,gamma)Na-23 reaction is the most uncertain process in the neon-sodium cycle of hydrogen burning. At temperatures relevant for... 
YIELDS | SUPER | INPUT | MULTIPLE POPULATIONS | THERMONUCLEAR REACTION-RATES | PHYSICS, NUCLEAR | GALACTIC GLOBULAR-CLUSTERS | NUCLEOSYNTHESIS | NUCLEAR ASTROPHYSICS | CAPTURE | AGB STARS
Journal Article
The European Physical Journal A, ISSN 1434-6001, 11/2014, Volume 50, Issue 11, pp. 1 - 10
The 22Ne(p,γ)23Na reaction takes part in the neon-sodium cycle of hydrogen burning. This cycle is active in asymptotic giant branch stars as well as in novae... 
Nuclear Physics, Heavy Ions, Hadrons | Nuclear Fusion | Physics | Particle and Nuclear Physics | Hydrogen
Journal Article
Physical Review Letters, ISSN 0031-9007, 09/2016, Volume 117, Issue 14
The O-17(p,alpha)N-14 reaction plays a key role in various astrophysical scenarios, from asymptotic giant branch stars to classical novae. It affects the... 
CNO ISOTOPES | REACTION-RATES | PHYSICS, MULTIDISCIPLINARY | RED GIANTS | GRAPHS | TABLES
Journal Article
PHYSICS LETTERS B, ISSN 0370-2693, 07/2004, Volume 591, Issue 1-2, pp. 61 - 68
We report on a new measurement of the N-14(p, gamma) O-15 capture cross section at E-p = 140 to 400 keV using the 400 kV LUNA accelerator facility at the... 
N-14(P,GAMMA)O-15 | MODELS | PHYSICS, MULTIDISCIPLINARY | STARS
Journal Article
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, ISSN 0370-2693, 07/2004, Volume 591, Issue 1-2, pp. 61 - 68
We report on a new measurement of the N(p,γ) O capture cross section at E =140 to 400 keV using the 400 kV LUNA accelerator facility at the Laboratori... 
26.20.+f | 24.30.-v | 24.50.+g
Journal Article
EPL, ISSN 0295-5075, 06/2018, Volume 122, Issue 5
When deriving resonance strengths using the thick-target yield approximation, for very narrow resonances it may be necessary to take beam energy straggling... 
PHYSICS, MULTIDISCIPLINARY | SETUP
Journal Article
EUROPEAN PHYSICAL JOURNAL A, ISSN 1434-6001, 09/2005, Volume 25, Issue 3, pp. 455 - 466
The astrophysical S(E) factor of N-14(p,gamma)O-15 has been measured for effective center-of-mass energies between E-eff = 119 and 367 keV at the LUNA facility... 
N-14(P,GAMMA)O-15 | ACCELERATOR | FACILITY | PHYSICS, NUCLEAR | GLOBULAR-CLUSTERS | AGE | PHYSICS, PARTICLES & FIELDS
Journal Article
Physics Letters B, ISSN 0370-2693, 03/2019, Volume 790, pp. 237 - 242
The O(p, ) N reaction affects the synthesis of N, O and F isotopes, whose abundances can be used to probe the nucleosynthesis and mixing processes occurring... 
Stellar hydrogen burning | Hydrostatic stellar nucleosynthesis
Journal Article
Physical Review C - Nuclear Physics, ISSN 0556-2813, 08/2008, Volume 78, Issue 2
Phys.Rev.C78:022802,2008 The rate of the hydrogen-burning carbon-nitrogen-oxygen (CNO) cycle is controlled by the slowest process, 14N(p,gamma)15O, which... 
Experimental Physics | Fysik | Physical Sciences | Naturvetenskap | Other Physics Topics | Annan fysik | Natural Sciences | Experimentell fysik
Journal Article
PHYSICS LETTERS B, ISSN 0370-2693, 01/2012, Volume 707, Issue 1, pp. 60 - 65
In the present work we report on a new measurement of resonance strengths omega gamma in the reaction Mg-25(p, gamma)Al-26 at E-cm = 92 and 189 key. This study... 
MASSIVE STARS | Proton-capture reaction | THERMONUCLEAR REACTION-RATES | PROTON-CAPTURE | PHYSICS, NUCLEAR | Reaction rate | AL-26 | Nuclear astrophysics | MG-25(P,GAMMA)AL-26 REACTION | Mg-Al cycle | EARLY SOLAR-SYSTEM | ASTRONOMY & ASTROPHYSICS | NUCLEOSYNTHESIS | THRESHOLD STATES | RESONANCES | PHYSICS, PARTICLES & FIELDS
Journal Article
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, ISSN 0370-2693, 03/2019, Volume 790, pp. 237 - 242
The O(p,α) N reaction affects the synthesis of N, O and F isotopes, whose abundances can be used to probe the nucleosynthesis and mixing processes occurring... 
Stellar hydrogen burning | Hydrostatic stellar nucleosynthesis
Journal Article
Physics Letters B, ISSN 0370-2693, 08/2019, Volume 795, pp. 122 - 128
The NeNa and the MgAl cycles play a fundamental role in the nucleosynthesis of asymptotic giant branch stars undergoing hot bottom burning. The reaction links... 
Experimental nuclear astrophysics | Stellar evolution | Underground nuclear physics | Hydrogen burning
Journal Article
Physical Review C - Nuclear Physics, ISSN 0556-2813, 01/2014, Volume 89, Issue 1
Background: The O-17( p,gamma)F-18 reaction affects the production of key isotopes ( e.g., F-18 and O-18) in the explosive hydrogen burning that powers... 
PRESOLAR GRAINS | REACTION-RATES | EVOLUTION | MODELS | CLASSICAL NOVAE | WHITE-DWARFS | S-FACTOR | PHYSICS, NUCLEAR | NUCLEOSYNTHESIS | INTERMEDIATE-MASS STARS | NUCLEAR ASTROPHYSICS
Journal Article
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