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AbstractAbstract
[en] The reactions 31P(p, γ)32S and 31P(p, α)28Si have been studied in the energy range 280-620 keV to investigate the influence of low-energy resonances on the stellar reaction rates. Several new resonances have been observed and the resonance strengths for both reaction channels have been determined. The reaction rates have been calculated from the present results and are compared with the results of Hauser-Feshbach calculations. (orig.)
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Journal Article
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Numerical Data
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ALPHA DECAY, ALPHA PARTICLES, BRANCHING RATIO, CAPTURE, DE-EXCITATION, ENERGY DEPENDENCE, EXCITATION FUNCTIONS, EXCITED STATES, EXPERIMENTAL DATA, GAMMA DECAY, GAMMA RADIATION, HAUSER-FESHBACH THEORY, ISOSPIN, KEV RANGE 100-1000, LEVEL WIDTHS, MULTI-NUCLEON TRANSFER REACTIO, NUCLEAR REACTION KINETICS, NUCLEAR REACTION YIELD, PARITY, PHOSPHORUS 31 TARGET, PHOTONS, PROTON REACTIONS, RESONANCE, SILICON 28, SPIN, STAR BURNING, STRENGTH FUNCTIONS, SULFUR 32, TEMPERATURE DEPENDENCE, THREE-NUCLEON TRANSFER REACTIO
ANGULAR MOMENTUM, BARYON REACTIONS, BOSONS, CHARGED PARTICLES, DATA, DECAY, DIRECT REACTIONS, ELECTROMAGNETIC RADIATION, ELEMENTARY PARTICLES, ENERGY LEVELS, ENERGY RANGE, ENERGY-LEVEL TRANSITIONS, EVEN-EVEN NUCLEI, FUNCTIONS, HADRON REACTIONS, HELIUM IONS, INFORMATION, IONIZING RADIATIONS, IONS, ISOTOPES, KEV RANGE, KINETICS, LIGHT NUCLEI, MASSLESS PARTICLES, NUCLEAR DECAY, NUCLEAR REACTIONS, NUCLEAR THEORY, NUCLEI, NUCLEON REACTIONS, NUMERICAL DATA, PARTICLE PROPERTIES, RADIATIONS, REACTION KINETICS, SILICON ISOTOPES, STABLE ISOTOPES, SULFUR ISOTOPES, TARGETS, TRANSFER REACTIONS
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