dc.contributor.author | Sharma, Shweta | |
dc.contributor.author | Ball, G. C. | |
dc.contributor.author | Bernier, Nikita | |
dc.date.accessioned | 2022-07-28T10:29:49Z | |
dc.date.available | 2022-07-28T10:29:49Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | Sharma, S. et al. (2022). High-precision half-life determination of 14O via direct β counting. The European Physical Journal A, 58, 83. https://doi.org/10.1140/epja/s10050-022- | en_US |
dc.identifier.issn | 1434-601X | |
dc.identifier.uri | https://doi.org/10.1140/epja/s10050-022-00730-w | |
dc.identifier.uri | http://hdl.handle.net/10566/7646 | |
dc.description.abstract | The half-life of the superallowed Fermi β+ emitter 14O was determined to high precision via a direct
β counting experiment performed at the Isotope Separator and Accelerator (ISAC) facility at TRIUMF. The result,
T1/2(
14O) = 70619.2(76) ms, is consistent with, but is more
precise than, the world average obtained from 11 previous
measurements. Combining the 14O half-life deduced in the
present work with the previous most precise measurements
of this quantity leads to a reduction in the overall uncertainty, by nearly a factor of 2. The new world average is
T1/2(
14O) = 70619.6(63) ms with a reduced χ2 value of 0.87
obtained from 8 degrees of freedom. | en_US |
dc.language.iso | en | en_US |
dc.publisher | Springer | en_US |
dc.subject | Astrophysics | en_US |
dc.subject | Physics | en_US |
dc.subject | Astronomy | en_US |
dc.subject | Science | en_US |
dc.title | High-precision half-life determination of 14O via direct β counting | en_US |
dc.type | Article | en_US |