Branches of {sup 33}S(p,{gamma}){sup 34}Cl at oxygen-neon nova temperatures
Journal Article
·
· Physical Review. C, Nuclear Physics
- Department of Physics, University of Washington, Seattle, Washington 98195-1560 (United States)
- Physik Department E12, Technische Universitaet Muenchen, D-85748 Garching (Germany)
Recent simulations of classical novae on oxygen-neon white-dwarf stars indicate that the isotopic ratio {sup 32}S/{sup 33}S has the potential to be a remarkable indicator of presolar grains of nova origin. The {sup 33}S(p,{gamma}){sup 34}Cl reaction influences this ratio directly by destroying {sup 33}S in novae. Additionally, {beta}-delayed {gamma} rays from the metastable state of {sup 34}Cl (t{sub 1/2}=32 min) have been suggested to be potential nova observables. We have measured the branches for known {sup 33}S(p,{gamma}){sup 34}Cl resonances that are activated at temperatures relevant to oxygen-neon novae. We provide the first reliable uncertainties on these branches and the first upper limits for several previously unmeasured branches.
- OSTI ID:
- 21499645
- Journal Information:
- Physical Review. C, Nuclear Physics, Journal Name: Physical Review. C, Nuclear Physics Journal Issue: 4 Vol. 83; ISSN 0556-2813; ISSN PRVCAN
- Country of Publication:
- United States
- Language:
- English
Similar Records
New {sup 34}Cl proton-threshold states and the thermonuclear {sup 33}S(p,{gamma}){sup 34}Cl rate in ONe novae
Improving the {sup 33}S(p,{gamma}){sup 34}Cl Reaction Rate for Models of Classical Nova Explosions
Journal Article
·
Wed Jul 15 00:00:00 EDT 2009
· Physical Review. C, Nuclear Physics
·
OSTI ID:21290019
Improving the {sup 33}S(p,{gamma}){sup 34}Cl Reaction Rate for Models of Classical Nova Explosions
Journal Article
·
Fri Oct 28 00:00:00 EDT 2011
· AIP Conference Proceedings
·
OSTI ID:21612046
Related Subjects
73 NUCLEAR PHYSICS AND RADIATION PHYSICS
BARYON REACTIONS
BETA DECAY RADIOISOTOPES
BETA-PLUS DECAY RADIOISOTOPES
BINARY STARS
BRANCHING RATIO
CHARGED-PARTICLE REACTIONS
CHLORINE 34
CHLORINE ISOTOPES
DATA COVARIANCES
DECAY
DIMENSIONLESS NUMBERS
DWARF STARS
ELECTROMAGNETIC RADIATION
ELEMENTS
ENERGY LEVELS
ERUPTIVE VARIABLE STARS
EXCITED STATES
FLUIDS
GAMMA DECAY
GAMMA RADIATION
GASES
HADRON REACTIONS
IONIZING RADIATIONS
ISOMERIC TRANSITION ISOTOPES
ISOTOPE RATIO
ISOTOPES
LIGHT NUCLEI
METASTABLE STATES
MINUTES LIVING RADIOISOTOPES
NEON
NONMETALS
NOVAE
NUCLEAR DECAY
NUCLEAR REACTIONS
NUCLEI
NUCLEON REACTIONS
ODD-ODD NUCLEI
OXYGEN
PROTON REACTIONS
RADIATIONS
RADIOISOTOPES
RARE GASES
RESONANCE
SECONDS LIVING RADIOISOTOPES
SIMULATION
STARS
SULFUR 33 TARGET
TARGETS
VARIABLE STARS
WHITE DWARF STARS
BARYON REACTIONS
BETA DECAY RADIOISOTOPES
BETA-PLUS DECAY RADIOISOTOPES
BINARY STARS
BRANCHING RATIO
CHARGED-PARTICLE REACTIONS
CHLORINE 34
CHLORINE ISOTOPES
DATA COVARIANCES
DECAY
DIMENSIONLESS NUMBERS
DWARF STARS
ELECTROMAGNETIC RADIATION
ELEMENTS
ENERGY LEVELS
ERUPTIVE VARIABLE STARS
EXCITED STATES
FLUIDS
GAMMA DECAY
GAMMA RADIATION
GASES
HADRON REACTIONS
IONIZING RADIATIONS
ISOMERIC TRANSITION ISOTOPES
ISOTOPE RATIO
ISOTOPES
LIGHT NUCLEI
METASTABLE STATES
MINUTES LIVING RADIOISOTOPES
NEON
NONMETALS
NOVAE
NUCLEAR DECAY
NUCLEAR REACTIONS
NUCLEI
NUCLEON REACTIONS
ODD-ODD NUCLEI
OXYGEN
PROTON REACTIONS
RADIATIONS
RADIOISOTOPES
RARE GASES
RESONANCE
SECONDS LIVING RADIOISOTOPES
SIMULATION
STARS
SULFUR 33 TARGET
TARGETS
VARIABLE STARS
WHITE DWARF STARS