1969
DOI: 10.1016/0375-9474(69)90721-0
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The ft value of the superallowed fermi beta decay 26mAl(β+)26Mg

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1971
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Cited by 47 publications
(8 citation statements)
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“…Consequently, a number of mostly pre-1970 measurements have been rejected because they were not analyzed with the "maximum-likelihood" method. The importance of using this technique for precision measurements was not recognized until that time [64] and, without access to the primary data, there is no way a new analysis can be applied retroactively. All rejected half-life • Pr67 ( 18 Ne)…”
Section: B Data Tablesmentioning
confidence: 99%
“…Consequently, a number of mostly pre-1970 measurements have been rejected because they were not analyzed with the "maximum-likelihood" method. The importance of using this technique for precision measurements was not recognized until that time [64] and, without access to the primary data, there is no way a new analysis can be applied retroactively. All rejected half-life • Pr67 ( 18 Ne)…”
Section: B Data Tablesmentioning
confidence: 99%
“…Al has an interesting level structure, in that it has a long lived (t 1/2 = 6.34 s) state only 228 keV above its ground state [1]. The β-decay of the ground state of 26 Al populates an excitation state in 26 Mg* which then emits a characteristic γ ray with an energy of 1.809 MeV.…”
Section: Introductionmentioning
confidence: 99%
“…Arguably the most studied γ-ray signature is the 1.809-MeV line from the β decay (t 1/2 = 7.2 × 10 5 y) of the J π = 5 + ground state of 26 Al ( 26g Al), a direct indication of the ongoing formation of 26 Al within our Galaxy. This signature is insensitive to 26 Al synthesized in its 0 + metastable state at 228 keV ( 26m Al), which β decays to the 26 Mg ground state (t 1/2 = 6.34 s [1]). Following inferences of 26 Al from meteoritic isotopic ratios [2] and the subsequent landmark astronomical detection of the 26g Al γ-ray signature [3], 26g Al has been the focus of increasingly sensitive measurements, aided by and driving the development of satellite-based γ-ray telescopes [4,5].…”
mentioning
confidence: 99%