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8B (66LA04)(See Energy Level Diagrams for 8B) GENERAL: See (FO58D, TA60L, IN62, NA63E, BA64I, BA64GG, GR64C, ST64). See also Table 8.18 [Table of Energy Levels] (in PDF or PS).
The beta decay leads mainly to 8Be*(2.9). Reported half lives are listed in Table 8.19 (in PDF or PS); taking τ1/2 = 0.774 sec and Q = 17.979 - 2.90, ft = 4.41 x 105 (BA65K). There is also observed a branch to a 8Be state at ~ 16.6 MeV; log ft = 2.9 (MA64D). See also (BA64GG) and 8Be.
Thresholds for production of slow neutrons are reported at E(3He) = 2.9661 ± 0.0017 MeV (DU58), 2.974 ± 0.010 MeV (FA59A), corresponding to the ground state of 8B, and at E(3He) = 4.16 ± 0.05 (DU58), 4.159 ± 0.030 MeV (FA59A), corresponding to an excited state at Ex = 0.789 ± 0.030 MeV with Γc.m. = 70 ± 40 keV. A threshold at 3.9 MeV reported by (DU58) is not confirmed by (FA59A). Neutron time-of-flight spectra at E(3He) = 4 to 9 MeV show groups corresponding to 8B(0) and 8B*(0.8), with forward-peaked angular distributions, and to a new state at Ex = 2.17 ± 0.05 MeV (DI63). At E(3He) = 4.5 to 5.3 MeV, time-of-flight spectra locate the first excited state at 0.767 ± 0.012 (FA65B), 0.783 ± 0.010 MeV (MC65E: Γ = 40 ± 10 keV). See also (MO63I).
The cross section for proton capture is 0.48 ± 0.18 μb at Ep = 0.80 MeV and 0.50 ± 0.20 μb at Ep = 1.40 MeV (KA60). The relevance of this reaction in stellar energy production is discussed by (FO58D, KA60, BA63DD, BA64I, PA64E). See also (CH61C).
See (AL50G).
See (SH52).
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