Measurement of the β-p emission of 20Mg and the breakout from the hot CNO cycle

Details Measurement of the β-p emission of 20Mg and the breakout from the hot CNO cycle Measurement of the β-p emission of 20Mg and the breakout from the hot CNO cycle

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1304..429w&link_type=abstract

EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (III): From Nuclei to Stars. AIP Conference Proceedings, Volume 1304, pp. 429-4

Astronomy and Astrophysics

Astrophysics

Excited States, Beta-Decay, Nuclear Fragmentation, Cherenkov Counters, Atomic Excitation And Ionization By Electron Impact, Weak-Interaction And Lepton Aspects, Projectile And Target Fragmentation, Cherenkov Detectors

Scientific paper

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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