Experimental study of {beta}-delayed proton decay of {sup 23}Al for nucleosynthesis in novae
- Department of Physics, University of Jyvaeskylae, P.O. Box 35 (YFL), FI-40014 Finland (Finland)
- Cyclotron Institute, Texas A and M University, College Station, Texas 77843-3366 (United States)
- Department of Physics, University of York, Heslington, York YO10 5DD (United Kingdom)
- School of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3JZ (United Kingdom)
The {beta}-delayed {gamma} and proton decay of {sup 23}Al has been studied with an alternative detector setup at the focal plane of the momentum achromat recoil separator MARS at Texas A and M University. We could detect protons down to an energy of 200 keV and determine the corresponding branching ratios. Contrary to results of previous {beta}-decay studies, no strong proton intensity from the decay of the isobaric analog state (IAS) of the {sup 23}Al ground state at E{sub x}=7803 keV in {sup 23}Mg was observed. Instead we assign the observed low-energy group E{sub p,c.m.}=206 keV to the decay from a state that is 16 keV below the IAS. We measured both proton and gamma branches from the decay of this state at E{sub x}=7787 keV in {sup 23}Mg, which is a very rare case in the literature. Combining our data with its measured lifetime, we determine its resonance strength to be {omega}{gamma}=1.4{sub -0.4}{sup +0.5} meV. The value is in agreement with older direct measurements, but disagrees with a recent direct measurement. This state is the most important resonance for the radiative proton capture {sup 22}Na(p,{gamma}){sup 23}Mg in some astrophysical environments, such as novae.
- OSTI ID:
- 21499634
- Journal Information:
- Physical Review. C, Nuclear Physics, Vol. 83, Issue 4; Other Information: DOI: 10.1103/PhysRevC.83.045808; (c) 2011 American Institute of Physics; ISSN 0556-2813
- Country of Publication:
- United States
- Language:
- English
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ALUMINIUM 23
ASTROPHYSICS
BETA DECAY
BRANCHING RATIO
CAPTURE
DELAYED PROTONS
GAMMA DECAY
GROUND STATES
ISOBARIC ANALOGS
KEV RANGE 100-1000
LIFETIME
MAGNESIUM 23
MEV RANGE
NOVAE
NUCLEOSYNTHESIS
PROTON REACTIONS
RECOILS
RESONANCE
SIMULATION
SODIUM 22 TARGET
ALKALINE EARTH ISOTOPES
ALUMINIUM ISOTOPES
BARYON REACTIONS
BARYONS
BETA DECAY RADIOISOTOPES
BETA-PLUS DECAY RADIOISOTOPES
BINARY STARS
CHARGED-PARTICLE REACTIONS
DECAY
DIMENSIONLESS NUMBERS
ELEMENTARY PARTICLES
ENERGY LEVELS
ENERGY RANGE
ERUPTIVE VARIABLE STARS
EVEN-ODD NUCLEI
FERMIONS
HADRON REACTIONS
HADRONS
ISOTOPES
KEV RANGE
LIGHT NUCLEI
MAGNESIUM ISOTOPES
MILLISECONDS LIVING RADIOISOTOPES
NUCLEAR DECAY
NUCLEAR REACTIONS
NUCLEI
NUCLEON REACTIONS
NUCLEONS
ODD-EVEN NUCLEI
PHYSICS
PROTONS
RADIOISOTOPES
SECONDS LIVING RADIOISOTOPES
STARS
SYNTHESIS
TARGETS
VARIABLE STARS