Published May 2010
| Version v1
Journal article
Resonance strength in 22Ne(p,γ)23Na from depth profiling in aluminum
Creators
- 1. National Institute of Standards and Technology, 100 Bureau Drive, Stop 8462, Gaithersburg, Maryland 20899-8462 (United States)
- 2. Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, North Carolina 27599, USA and Triangle Universities Nuclear Laboratory, Durham, North Carolina 27708 (United States)
Description
A novel method for extracting absolute resonance strengths has been investigated. By implanting 22Ne ions into a thick aluminum backing and simultaneously measuring the 22Ne+p and 27Al+p reactions, the strength of the Erlab=479 keV resonance in 22Ne(p,γ)23Na was determined to be ωγ=0.524(51) eV. This result has significantly reduced uncertainties compared to earlier work. Our results are important for the absolute normalizations of resonance strengths in the 22Ne(p,γ)23Na hydrogen-burning reaction and in the 22Ne+α s-process neutron-source reactions.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 81
- Journal Issue
- 5
- Journal Page Range
- p. 055804-055804.8
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41117817
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ALUMINIUM; ALUMINIUM 27; EV RANGE; GAMMA DECAY; HYDROGEN BURNING; ION IMPLANTATION; ION-ATOM COLLISIONS; IONS; KEV RANGE; NEON 22 TARGET; NEUTRON SOURCES; PROTON REACTIONS; RESONANCE; S PROCESS; SIMULATION; SODIUM 23
- Descriptors DEC
- ALUMINIUM ISOTOPES; ATOM COLLISIONS; BARYON REACTIONS; CHARGED PARTICLES; CHARGED-PARTICLE REACTIONS; COLLISIONS; DECAY; ELEMENTS; ENERGY RANGE; EVOLUTION; HADRON REACTIONS; ION COLLISIONS; ISOTOPES; LIGHT NUCLEI; METALS; NUCLEAR DECAY; NUCLEAR REACTIONS; NUCLEI; NUCLEON REACTIONS; ODD-EVEN NUCLEI; PARTICLE SOURCES; RADIATION SOURCES; SODIUM ISOTOPES; STABLE ISOTOPES; STAR BURNING; STAR EVOLUTION; TARGETS
Optional Information
- Notes
- (c) 2010 The American Physical Society