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AbstractAbstract
[en] In the astrophysically important reaction 19Ne(p,γ)20Na, the rate is dominated by a single key resonance at 450 keV above the proton-emission threshold in 20Na. Throughout the last few decades many experiments have been performed aimed at finding the identity of this state. Despite this, the spin-parity of the key resonant state is still up for debate. The present paper describes a new experiment studying the β-delayed proton decay of 20Mg aimed at solving this issue.
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Source
Carpathian summer school of physics - Exotic nuclei and nuclear/particle astrophysics (III): From nuclei to stars; Sinaia (Romania); 20 Jun - 3 Jul 2010; (c) 2010 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
Record Type
Journal Article
Literature Type
Conference
Journal
Country of publication
ALKALINE EARTH ISOTOPES, ANGULAR MOMENTUM, BARYON REACTIONS, BARYONS, BETA DECAY RADIOISOTOPES, BETA-PLUS DECAY RADIOISOTOPES, CHARGED-PARTICLE REACTIONS, DECAY, ELECTRON CAPTURE RADIOISOTOPES, ELEMENTARY PARTICLES, ENERGY LEVELS, ENERGY RANGE, EVEN-EVEN NUCLEI, EVEN-ODD NUCLEI, FERMIONS, HADRON REACTIONS, HADRONS, ISOTOPES, KEV RANGE, LIGHT NUCLEI, MAGNESIUM ISOTOPES, MEASURING INSTRUMENTS, MILLISECONDS LIVING RADIOISOTOPES, NEON ISOTOPES, NUCLEAR DECAY, NUCLEAR REACTIONS, NUCLEI, NUCLEON REACTIONS, NUCLEONS, ODD-ODD NUCLEI, PARTICLE PROPERTIES, PROTONS, RADIATION DETECTORS, RADIOISOTOPES, SECONDS LIVING RADIOISOTOPES, SODIUM ISOTOPES, STAR BURNING
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