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16N (1959AJ76)(See the Energy Level Diagram for 16N) GENERAL: See also Table 16.1 [Table of Energy Levels] (in PDF or PS). Theory: See (1954FL1A, 1956KA1C, 1957EL1B).
From the character of the beta decay, it is concluded that 16N(0) has Jπ = 2-. See 16O.
See (1958AL1D).
The cross section for this reaction has been measured from E(7Li) = 1.1 to 2.0 MeV. At the higher energy it is approximately 1 mb (1957NO17).
Not reported.
At Ed = 1.16 MeV, the cross section is ≲ 0.1 mb (1957BO04). At Ed = 2.0 MeV, σ ≤ 0.6 mb (1956DO37).
The excitation function has been studied from Ed = 0.6 to 3.0 MeV (1954RI1B, 1956DO37). Resonances are observed at 2.0, 2.45 and 2.7 MeV, with c.m. widths of 270, 190 and 165 keV, respectively, corresponding to 16N*(12.2, 12.62, 12.8 MeV) (1956DO37). See also (1950HU72, 1954RI1B) and 15C.
See (1950HU72).
Not reported.
Not reported.
Not reported.
See (1953CU1D).
The thermal cross section is 24 ± 8 μb (1958HU18), 80 ± 30 μb (1952FE1A).
The total cross section has been measured for En = 2.8 to 3.3 MeV: a resonance is observed at En ≈ 2.95 MeV. σmax = 4 b, Γ = 140 ± 40 keV, corresponding to Ex ≈ 5.26 MeV, J = 2- or 3± (1956BA1A).
See (1948JE03).
Levels derived from observed proton groups and γ-rays are listed in Table 16.2 [Levels of 16N from 15N(d, p)16N] (in PDF or PS). Gamma transitions are shown in the inset of Fig. 31 (Energy Level Diagram of 16N). Even at Ed = 2.7 MeV, the stripping angular distribution patterns to the low-lying states are well-developed, and the theory yields quite good fits (1956ZI1A, 1957WA01). Shell-model theory in intermediate coupling predicts a close group of 4 levels within about 700 keV, with J = 0, 1, 2, 3, odd parity (order uncertain), arising from the configurations p1/2-1s1/2 and p1/2-1d5/2. Levels from p1/2-1d3/2 should lie several MeV higher (1953IN1A, 1957EL1B). These results are strikingly confirmed by the experimental evidence. The ground state is assigned J = 2- on the basis of the β-decay (see 16N(β-)16O). The first excited state may have J = 0- or 1- from the stripping pattern; however, the half-life τ1/2 = 6.7 ± 0.5 μsec (1957FR56), 5.43 ± 0.22 μsec (1959ZI18) is much too long for dipole radiation, and J = 0- is indicated (1957WI1B). The third excited state (Ex = 392 keV), again limited to J = 0- or 1- by the stripping pattern, decays to both 16N(0) and 16N*(0.12); J = 0- is therefore excluded and J = 1- indicated. Of the possibilities J = 1-, 2-, 3- for the second excited state, 16N*(0.285), J = 1- is rendered unlikely by the low intensity of γ-decay to the second excited state and by the absence of an ln = 0 component in the stripping pattern (1956ZI1A, 1957WA01, 1957WI1B). The assignment J = 3- is strongly favored by the (p - γ) angular correlation (1957FR56). The observed γ-branching of 16N*(0.395) is in accord with the theory, which predicts lifetimes in the range 1 to 7 × 10-11 sec. A considerable enhancement through collective excitation is required to account for the lifetime of the first excited state. The reduced neutron widths are expected to be of the order of the single-particle limit. Calculation of level shifts and comparison of observed reduced widths suggests that the 16O* analogues to the first four states of 16N are 16O*(12.95, 12.78, 13.24, 13.09 MeV) (1957EL1B): see also (1957WI1B) and 15N(p, p)15N.
Not reported.
Not reported.
The possibility that 16N might have a long-lived (≈ sec) isomeric state has been examined, with negative result (1956TO1A). See also (1952LI24) and 17O.
Not reported.
Not reported.
Not reported.
Not reported.
Alpha groups are observed at Ed = 0.85 MeV corresponding to 16N*(0, 116 ± 6, 300 ± 12, 391 ± 12 keV). No other states are observed below Ex = 1.24 MeV (1955PA50). See also (1957BO04) and 20F.
At En = 4.87 MeV, an α-group has been observed with Q = -1.77 ± 0.15 MeV, probably corresponding to a transition to one or more excited states of 16N (1955JA18). See also (1956TO1A) and 20F.
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