gamma. width of the unbound 5. 17 MeV level of sup 14 O and the hot'' CNO cycle
Journal Article
·
· Physical Review (Section) C: Nuclear Physics; (USA)
- Physics Department, University of Washington, Seattle, Washington 98195 (US)
We have measured the {gamma}-ray branching ratio {Gamma}{sub {gamma}}/{Gamma} of the unbound 5.17 MeV first excited state in {sup 14}O using the {sup 12}C({sup 3}He,{ital n}{gamma}) reaction at {ital E}{sub {sup 3}He}=9.35 MeV. We detected coincidences between {ital n}{sub 1} neutrons populating the {sup 14}O state and 5.17 MeV {gamma} rays from its decay, and obtained {Gamma}{sub {gamma}}/{Gamma}=(7.2{plus minus}3.5){times}10{sup {minus}5}. When combined with the known total width {Gamma}=38.1{plus minus}1.8 keV, our branching ratio corresponds to {Gamma}{sub {gamma}}=2.7{plus minus}1.3 eV. We use this {gamma}-ray width, together with previously measured nonresonant {sup 13}C({ital p},{gamma}{sub 1}) data, to find the {sup 13}N({ital p},{gamma}) reaction rate at astrophysical energies, thereby determining the stellar environments where hydrogen burning through hot'' or {beta}-limited CNO cycle can occur.
- OSTI ID:
- 5015914
- Journal Information:
- Physical Review (Section) C: Nuclear Physics; (USA), Journal Name: Physical Review (Section) C: Nuclear Physics; (USA) Vol. 40:5; ISSN 0556-2813; ISSN PRVCA
- Country of Publication:
- United States
- Language:
- English
Similar Records
Gamma decay of the 5. 17-MeV level in sup 14 O and the hot CNO cycle
Total width of the 5. 17 MeV 1/sup -/ state in /sup 14/O and the hot-CNO cycle
Gamma width of [sup 14]O[sup *](5. 17 MeV) and the stellar [sup 13]N([ital p],[gamma])[sup 14]O reaction rate
Thesis/Dissertation
·
Sat Dec 31 23:00:00 EST 1988
·
OSTI ID:6047903
Total width of the 5. 17 MeV 1/sup -/ state in /sup 14/O and the hot-CNO cycle
Journal Article
·
Thu Feb 28 23:00:00 EST 1985
· Phys. Rev. C; (United States)
·
OSTI ID:6129351
Gamma width of [sup 14]O[sup *](5. 17 MeV) and the stellar [sup 13]N([ital p],[gamma])[sup 14]O reaction rate
Journal Article
·
Tue Jun 01 00:00:00 EDT 1993
· Physical Review, C (Nuclear Physics); (United States)
·
OSTI ID:6581498
Related Subjects
651320* -- Nuclear Properties & Reactions
A=6-19
Experimental
73 NUCLEAR PHYSICS AND RADIATION PHYSICS
ASTROPHYSICS
BARYONS
BETA DECAY RADIOISOTOPES
BETA-PLUS DECAY RADIOISOTOPES
BRANCHING RATIO
CARBON 12 TARGET
CHARGED-PARTICLE REACTIONS
CNO CYCLE
COINCIDENCE SPECTROMETRY
COMPOUND-NUCLEUS REACTIONS
CROSS SECTIONS
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
ELEMENTS
ENERGY LEVELS
ENERGY RANGE
EVEN-EVEN NUCLEI
FERMIONS
GAMMA RADIATION
HADRONS
HELIUM 3 REACTIONS
HYDROGEN
IONIZING RADIATIONS
ISOTOPES
LIGHT NUCLEI
MEV RANGE
MEV RANGE 01-10
MINUTES LIVING RADIOISOTOPES
NEUTRONS
NONMETALS
NUCLEAR REACTIONS
NUCLEI
NUCLEONS
OXYGEN 14
OXYGEN ISOTOPES
RADIATIONS
RADIOISOTOPES
STAR BURNING
TARGETS
A=6-19
Experimental
73 NUCLEAR PHYSICS AND RADIATION PHYSICS
ASTROPHYSICS
BARYONS
BETA DECAY RADIOISOTOPES
BETA-PLUS DECAY RADIOISOTOPES
BRANCHING RATIO
CARBON 12 TARGET
CHARGED-PARTICLE REACTIONS
CNO CYCLE
COINCIDENCE SPECTROMETRY
COMPOUND-NUCLEUS REACTIONS
CROSS SECTIONS
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
ELEMENTS
ENERGY LEVELS
ENERGY RANGE
EVEN-EVEN NUCLEI
FERMIONS
GAMMA RADIATION
HADRONS
HELIUM 3 REACTIONS
HYDROGEN
IONIZING RADIATIONS
ISOTOPES
LIGHT NUCLEI
MEV RANGE
MEV RANGE 01-10
MINUTES LIVING RADIOISOTOPES
NEUTRONS
NONMETALS
NUCLEAR REACTIONS
NUCLEI
NUCLEONS
OXYGEN 14
OXYGEN ISOTOPES
RADIATIONS
RADIOISOTOPES
STAR BURNING
TARGETS