1992
DOI: 10.1007/bf01291509
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Beta-delayed two-proton decay of39Ti

Abstract: The beta-delayed two-proton decay of the T~ = -5/2 nuclide 39Ti has been observed. The a9Sc isobaric analog state has been calculated to lie at 8.82 MeV using the measured two-proton sum energy of 4750+40 keV for its decay to the 37K ground state. Combining this excitation energy with a Coulomb displacement energy calculation has lowered the energy available for ground state two-proton emission of 39Ti from 760 to 530 keV.

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Cited by 31 publications
(11 citation statements)
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“…The limited statistics of the present work as well as of the work from Détraz et al [17] and Moltz et al [18] does not allow for a detailed comparison of the energy spectra. However, from the proton spectrum in figure 3a, it seems to be likely that the peak at (4880 ± 40) keV (marked as This energy is 130 keV higher than in the work of Moltz et al [18] and leads to an excitation energy of the isobaric analogue state (IAS) in 39 Sc of (8.96 ± 0.06) MeV.…”
Section: The Decay Of 39 Timentioning
confidence: 64%
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“…The limited statistics of the present work as well as of the work from Détraz et al [17] and Moltz et al [18] does not allow for a detailed comparison of the energy spectra. However, from the proton spectrum in figure 3a, it seems to be likely that the peak at (4880 ± 40) keV (marked as This energy is 130 keV higher than in the work of Moltz et al [18] and leads to an excitation energy of the isobaric analogue state (IAS) in 39 Sc of (8.96 ± 0.06) MeV.…”
Section: The Decay Of 39 Timentioning
confidence: 64%
“…However, from the proton spectrum in figure 3a, it seems to be likely that the peak at (4880 ± 40) keV (marked as This energy is 130 keV higher than in the work of Moltz et al [18] and leads to an excitation energy of the isobaric analogue state (IAS) in 39 Sc of (8.96 ± 0.06) MeV. From this result, we deduce a mass excess for this analog state of ∆m = (−5210 ± 85) keV.…”
Section: The Decay Of 39 Timentioning
confidence: 65%
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“…However, for some nuclei at the drip line, even more exotic decay branches are possible. After the first observation of β-delayed two-proton emission for 22 Al [2], 6 more β2p emitters have been found: 26 P [3], 35 Ca [4], 31 Ar [5], 27 S [6], 39 Ti [7], and 43 Cr [8]. For 31 Ar, a β-delayed three-proton emission has been reported [9a] D. Bazin et al.…”
Section: Introductionmentioning
confidence: 97%
“…Though two separate gas ∆E -E proton identifications had been planned for each event of interest to further reduce the beta-particle background [12], these 3 He measurements showed that there were problems with the gas gains of the ∆E1 detectors, so that only a single identification of protons using the gas ∆E2 -(Si) E coincidences was utilized. (However, the quality of the gas ∆E2 -(Si) E identifications alone was quite good and was similar to that shown in Figure 3d of [14] for many of the telescopes. )…”
mentioning
confidence: 78%