1992
DOI: 10.1103/physrevc.46.r833
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β-delayed proton decay ofMg20and its astrophysical implications

Abstract: We have studied the P-delayed proton decay of 2OMg to search for the 2645 keV state in t Na. This state is of astrophysical interest, because any proton capture through this state would dominate the stellar reaction rate of the reaction ' Ne(p, y) Na. This reaction determines the break out from the hot CNO cycle. Several proton groups have been observed and their logft values have been determined. No protons from the 2645 keV state were seen and a lower limit of logft~5. 85 has been established. The impact of … Show more

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Cited by 35 publications
(24 citation statements)
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“…The present excitation energy of the lowest T = 2 state is 27 keV (1.9 standard deviations) lower than the value of 6525±14 keV from the most recent data evaluation [3], which was based on several measurements of 20 Mg betadelayed proton emission [18,24,25]. The present value is also 28 times more precise.…”
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confidence: 61%
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“…The present excitation energy of the lowest T = 2 state is 27 keV (1.9 standard deviations) lower than the value of 6525±14 keV from the most recent data evaluation [3], which was based on several measurements of 20 Mg betadelayed proton emission [18,24,25]. The present value is also 28 times more precise.…”
mentioning
confidence: 61%
“…For example, we anticipate that this method could be applied to the decays of 24 Si, 28 S, 36 Ca, and so on, given sufficient rare-isotope production and a sufficiently sensitive gamma-ray spectrometer.…”
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confidence: 99%
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“…It turned out that, due to the low implantation rate of about one 20 Na per second and of about three of each of the other isotopes per second, only a small contamination from the 20 Na activity might be possible due to its long half-life and its high branching ratios of its main α groups. The energy spectra of β-delayed protons were calibrated with the known β-delayed proton or α emitters 20 Na [15], 24 Si [16], 21 Mg [17], and 20 Mg [18,19]. 23 Si β-delayed protons have been measured in both the last silicon detector and the MSGC.…”
Section: Experimental Techniquementioning
confidence: 99%