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11Li (1990AJ01)(See the Isobar Diagram for 11Li) GENERAL: See also (1985AJ01) and Table 11.1 [Table of Energy Levels] (in PDF or PS). The mass excess is 40.94 ± 0.08 MeV (1875TH08), 40.78 ± 0.12 MeV (1988WO09). A.H. Wapstra suggests (private communication) 40.85 ± 0.08 MeV and we adopt this value. 11Li is then bound with respect to 9Li + 2n by 247 ± 80 keV and with respect to 10Li + n by 1050 ± 260 keV [see the masses of 9Li and 10Li in (1988AJ01)]. The magnetic moment of 11Li is μ = 3.6673 ± 0.0025 nm (1987AR22). This value requires J = 3/2 (1987AR22). Negative parity is certain from systematics. The interaction nuclear radius of 11Li is 3.16 ± 0.11 fm (1988TA10, 1985TA18), E = 790 MeV/A; [see also for derived nuclear matter, charge and neutron matter r.m.s. radii]. 11Li has a much larger radius than other neighboring nuclei suggesting either a large deformation and/or a long tail in the matter distribution in 11Li (1985TA18). See (1988SA2P) and (1987MI38, 1987TAZU, 1989TA1K). Charge radius and matter radius calculations in the 0ℏω and (0+2)ℏω model spaces predict a gradual increase in matter radii with increasing A and do not support the idea of a neutron halo in 11Li (1988POZS; prelim.). See, however, (1988TA1A). Fragmentation cross sections of 11Li into 9Li, 8Li, 8He, 7Li, 6Li and 6He have been studied by (1988KO10) [see for a discussion of neutron halos]. See also (1988TA1A, 1989KO1P). See also (1986DU11, 1988ST06), (1986AN07, 1988HA1Q, 1988TA1C, 1989AJ1A) and (1985SA32, 1986EL1A, 1986SA30, 1987HA30, 1987SH1K, 1988BE09, 1988BE1O, 1988JO1C, 1988LO1C, 1988UC03, 1989BA1T, 1989BE03; theor.).
Reported half-life measurements are 8.5 ± 0.2 ms (1974RO31), 8.83 ± 0.12 ms (1981BJ01), 7.7 ± 0.6 ms (1986CU01). We adopt 8.5 ± 0.2 ms. The β-decay is complex and the evidence is not unambiguous. It involves delayed n, t and α emission. Most of the decay (approximately 97%) takes place to low-lying states in 11Be [but it is not clear which are involved]. All but 11Be*(0, 0.32) are unstable with respect to neutron emission: see (1985AJ01). A 2.9% branch is reported to 11Be*(10.59) which then decays by neutron emission (possibly to 10Be*(9.4)) and then delayed α-particles [(0.90 ± 0.05)%] are reported to 6He or the decay is via 2n + 2α[(2.0 ± 0.6)%] (1981LA11). A (0.30 ± 0.05)% branch is reported to a state in 11Be at approximately18.5 MeV (Γ0.5 MeV) which has three modes of decay: triton emission to 8Li*(0, 0.98) [(0.010 ± 0.004)%], (α + n)-emission to 6He[(0.10 ± 0.03)%] and 3n emission [(0.20 ± 0.05%] involving 10Be*(11.76) (1981LA11, 1984LA27). [Comment: In view of the importance of understanding very neutron rich light nuclei it is necessary to determine the parameters (and the location) of the excited states of 11Be with Ex is approximately equal to 12 MeV. One could then hope to unravel the β- decay evidence.] See also 6He, 8Li and 10Be in (1988AJ01), Table 11.2 (in PDF or PS) in (1985AJ01), (1985HA1T, 1985HA1K) and (1984LI1N, 1988JO1C; theor.).
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