6533b870fe1ef96bd12cf02f
RESEARCH PRODUCT
Measurement of the 2+→0+ ground-state transition in the β decay of F20
B. A. BrownM. MunchM. VilenAri JokinenTommi EronenH. O. U. FynboIain MooreOlof TengbladKarlheinz LangankeKarlheinz LangankeL. CaneteAnu KankainenM. ReponenOliver S. KirsebomOliver S. KirsebomS. VinalsPankaj S. JoshiJuha ÄYstöGabriel Martínez-pinedoGabriel Martínez-pinedoA. KhanamA. KhanamHeikki PenttiläM. HukkanenD. G. JenkinsWladyslaw Henryk TrzaskaJoel KostensaloJ. D. OvejasJouni SuhonenJ. A. SwartzTimo EnqvistJ. CederkällK. RiisagerPasi KuusiniemiD. F. StrömbergD. F. StrömbergR. P. De GrooteP. C. SrivastavaIlkka PohjalainenS. GeldhofDmitrii NesterenkoE. BodewitsP. SchotanusK. AndersenSami Rinta-antilaA. De Roubinsubject
Physics010308 nuclear & particles physicsBranching fractionDegenerate energy levelsDetectorchemistry.chemical_element01 natural sciences7. Clean energychemistry0103 physical sciencesHigh Energy Physics::ExperimentAtomic physics010306 general physicsGround stateCarbonStellar evolutionBeam (structure)FOIL methoddescription
We report the first detection of the second-forbidden, nonunique, 2+→0+, ground-state transition in the β decay of F20. A low-energy, mass-separated F+20 beam produced at the IGISOL facility in Jyvaskyla, Finland, was implanted in a thin carbon foil and the β spectrum measured using a magnetic transporter and a plastic-scintillator detector. The β-decay branching ratio inferred from the measurement is bβ=[0.41±0.08(stat)±0.07(sys)]×10-5 corresponding to logft=10.89(11), making this one of the strongest second-forbidden, nonunique β transitions ever measured. The experimental result is supported by shell-model calculations and has significant implications for the final evolution of stars that develop degenerate oxygen-neon cores. Using the new experimental data, we argue that the astrophysical electron-capture rate on Ne20 is now known to within better than 25% at the relevant temperatures and densities. (Less)
year | journal | country | edition | language |
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2019-12-24 | Physical Review C |