A=14N (1981AJ01)

A recent measurement of the (5.83 → 5.11) γ-ray in reaction (b), E_γ = 728.34 ± 0.10 keV, leads to E_x = 5834.23 ± 0.21 keV (1981KO08) and E.K. Warburton, private communication. See also (1976AJ04).

2. ⁹Be(¹⁰B, αn)¹⁴N Q_m = 10.040

See (1979CH22).

3. ¹⁰B(α, n)¹³N Q_m = 1.060 E_b = 11.6133

Observed resonances are displayed in Table 14.13 (in PDF or PS). See also (1976AJ04).

4. ¹⁰B(α, p)¹³C Q_m = 4.0626 E_b = 11.6133

Excitation functions have been measured to E_α = 26 MeV. Observed resonances are displayed in Table 14.13 (in PDF or PS). (1975WI04) has expanded the angular distributions of the p₀ → p₃ groups into Legendre polynomials and fitted the coefficients at the resonances corresponding to ¹⁴N*(13.16, 13.24, 13.67, 13.76) obtaining J^π = 1⁺, 2^-, 2 or 3⁺, and 1, respectively, for these states. (1975WI04) also finds that a surprising proportion of states have a higher cross section for neutron than for proton emission: the fluctuations of σ_n/σ_p at low E_α suggest sizable isospin impurities in the ¹⁴N states. See also (1970AJ04, 1976AJ04).

5. ¹⁰B(α, d)¹²C Q_m = 1.3408 E_b = 11.6133

Excitation curves have been measured at E_α up to 27 MeV [see (1970AJ04, 1976AJ04)] and (1975VA19: E_α = 15 to 25 MeV; d₀, d₁). The low energy resonances are exhibited in Table 14.13 (in PDF or PS). At the higher energies the yield curves are fairly smooth although (1975VA19) show broad resonances in the d₁ and d₀ yields corresponding to ¹⁴N*(23, 25) respectively, and at θ = 170° (1975SP04) report a sharp rise in the 15.1 MeV γ yield ≈ 1 MeV above the ¹²C*(15.1) + p + n threshold, a channel which is not isospin forbidden. See also (1976LE1K).

6. ¹⁰B(α, α)¹⁰B E_b = 11.6133

The yield of α-particles [and of 0.7 MeV γ-rays for E_α = 2.1 to 3 MeV] has been measured for E_α to 30 MeV [see (1976AJ04)] and for E_α = 30 to 50.6 MeV by (1976BE1M; α₀). Observed resonances are displayed in Table 14.13 (in PDF or PS). In addition to two strong resonances in the α₀ yields at E_α = 2.21 and 4.26 MeV (¹⁴N*(13.19, 14.66)), two other states (¹⁴N*(13.72, 14.25)) are required to fit the data: an R-matrix calculation leads to J^π = 3⁺, 1⁺ [see, however, (1975WI04)], 3⁺ and 2^- for ¹⁴N*(13.19, 13.72, 14.25, 14.66) (1973MO15). A strong resonance at E_α = 5.0 ± 0.1 MeV is reported in the reaction cross section for E_α = 4.0 to 9.0 MeV (1976GR1F; abstract): it is suggested that J^π = 6⁺.

7. ¹⁰B(⁶Li, d)¹⁴N Q_m = 10.140

At E(⁶Li) = 5 MeV ¹⁴N*(0, 3.95, 4.92, 5.11, 5.69, 5.83, 6.20, 6.44, 7.03, 7.97, 8.49, 8.98, 9.12, 9.39, 9.70, 10.10, 10.43 (T = 1, weakly populated), 11.06) are populated ((1966MC05), and private communication). (1975FO01) have examined ¹⁴N*(9.13) in detail and conclude that it is a closely spaced doublet of which one member is populated in ¹³C(p, γ) and has been assigned J^π = 2^-, and the other member, populated here, has J^π = 3⁺. This assignment is based on a DWBA analysis of the angular distributions at E(⁶Li) = 16.5 and 21.0 MeV which shows the contributions of several L values and, in particular, L = 0. For γ branching ratios see Table 14.12 (in PDF or PS) of (1976AJ04). See also reaction 22.

8. ¹⁰B(⁷Li, t)¹⁴N Q_m = 9.147

At E(⁷Li) = 24 MeV angular distributions of the tritons to ¹⁴N*(3.95, 5.83, 6.44, 8.96, 9.13, 10.06, 10.81, 12.79 + 12.83, 13.03, 15.26) have been studied by (1977KO27). ¹⁴N*(4.91, 5.11, 5.69, 6.20, 7.03, 7.97, 8.49, 8.98, 9.39, 11.04, 11.05, 11.52, 12.41) are also populated (1977KO27).

9. (a) ¹¹B(³He, γ)¹⁴N Q_m = 20.7358 E_b = 20.7358
(b) ¹¹B(³He, n)¹³N Q_m = 10.182
(c) ¹¹B(³He, p)¹³C Q_m = 13.1851
(d) ¹¹B(³He, d)¹²C Q_m = 10.4634
(e) ¹¹B(³He, t)¹¹C Q_m = -2.001
(f) ¹¹B(³He, ³He)¹¹B
(g) ¹¹B(³He, α)¹⁰B Q_m = 9.1226
(h) ¹¹B(³He, ⁶Li)⁸Be Q_m = 4.5702

The capture γ-rays [reaction (a)] have been studied at E(³He) = 0.9 to 2.6 MeV (1970BL10; γ₀; θ = 0° and 90°). When the barrier penetration factor has been removed a single resonance is observed at E(³He) ≈ 1.4 MeV [¹⁴N*(21.8)], Γ_c.m. = 0.65 MeV. The higher energy work quoted in (1976AJ04) has not been published.

The excitation function for reaction (b) has been measured for E(³He) = 1.5 to 18 MeV [see (1976AJ04)] and 5.0 to 11.5 MeV (1977DA18; n₀). A broad peak at E(³He) = 4.15 MeV may indicate the existence of ¹⁴N*(24), Γ ≈ 1 MeV (1966DI04).

Yield curves for protons [reaction (c)] have been measured for E(³He) = 3.0 to 5.5 MeV (p₀, p₁, p₁ + p₂ + p₃): they are rather featureless (1959HO01). This is also true for the ground state deuterons of reaction (d) in the same energy interval (1959HO01). Yield curves for reaction (e) have been measured for E(³He) = 6 to 30 MeV: see (1976AJ04). See also ¹³C and ¹³N, and ¹¹B, ¹¹C, ¹²C in (1980AJ01).

The excitation functions for α-particle groups [reaction (g)] have been measured for E(³He) = 0.9 to 5.5 MeV: see (1976AJ04). No significant resonance behavior is seen except for the α₂ group which, in the 15° excitation function, exhibits a resonance at E(³He) = 4 MeV, Γ ≈ 1 MeV (1965FO06). See also ¹⁰B in (1979AJ01).

The excitation function for reaction (h) to ⁶Li_g.s. + ⁸Be_g.s. has been measured for E(³He) = 1.4 to 5.8 MeV: no pronounced structure is observed (1967YO02). At E(³He) = 25.20 to 26.25 MeV the excitation functions for the transitions to ⁸Be*(0, 16.63, 16.91, 17.64) are smooth, indicating a predominantly direct reaction mechanism (1974DE25).

10. ¹¹B(α, n)¹⁴N Q_m = 0.1580

Angular distributions have been measured for E_α to 13.9 MeV [see (1970AJ04, 1976AJ04)] and at E_α = 2.05 MeV (1977NI03). See also ¹⁵N and (1976EP1A, 1980DO1C; astrophys.).

11. ¹¹B(⁶Li, t)¹⁴N Q_m = 4.9418

See (1970AJ04).

12. ¹¹B(¹¹B, ⁸Li)¹⁴N Q_m = -6.475

At E(¹¹B) = 114 MeV the relatively strongly populated states are ¹⁴N*(5.83, 8.96, 12.8) [J^π = 3^-, 5⁺, 4⁺] (1974AN36).

13. ¹²C(d, γ)¹⁴N Q_m = 10.27240

At E_d = 1.5 MeV the capture cross section is < 1μb (1955AL16). [The other work quoted in (1976AJ04) has not been published.]

14. (a) ¹²C(d, n)¹³N Q_m = -0.2812 E_b = 10.27240
(b) ¹²C(d, p)¹³C Q_m = 2.7218

Resonances in the yields of neutrons and protons are displayed in Table 14.14 (in PDF or PS). Measurements of the yields of neutrons (to E_d = 17 MeV) and of protons (to E_d = 14.7 MeV) are listed in Tables 14.11 (in PDF or PS) (1970AJ04) and 14.16 (in PDF or PS) (1976AJ04). The yield of n₀ has also been measured by (1976WA1L: E_d = 5.5 to 12.5 MeV). This preliminary work is characterized by a broad bump at E_d ≈ 7 MeV and by a somewhat sharper one at E_d ≈ 9 MeV (1976WA1L). For angular distributions see ¹³C, ¹³N. For spallation measurements see (1978AZ1E, 1978DU1B).

The vector analyzing power and the 0° transverse vector polarization transfer coefficient, K^y'_y(0°) have been measured for E_d-bar = 5.7 to 9.7 MeV [n₀, n₁]. The values of K^y'_y are large, close to the maximum value of 2/3, consistent with a model of the neutron as a simple spectator in the reaction (1976TE03). K^y'_y(0°) has also been measured for 5 < E_d-bar < 12 MeV (1976WA1L; prelim.; n₀, n₁). Other recent measurements are those of the tensor polarization power for E_d-bar = 9 to 11 MeV (1977DR1F; p; prelim.) and the vector analyzing power at E_d-bar = 11 MeV (1976KR1B; n₀, n₁; prelim.). See also (1979SI07). For the earlier polarization measurements of neutrons (to E_d = 51.5 MeV) and of protons (to E_d = 51 MeV) see the listings in Table 14.12 (in PDF or PS) (1970AJ04) and 14.17 (in PDF or PS) (1976AJ04).

See also (1974LO1B, 1977HA1P, 1977SE1C, 1977SE09), (1977YO1F, 1977YO1G; applications) and (1975BO58, 1976SA04, 1978HA1Q, 1979SE04; theor.).

15. ¹²C(d, d)¹²C E_b = 10.27240

Reported resonances are displayed in Table 14.14 (in PDF or PS). Yield measurements of d₀ up to E_d = 26.5 MeV are listed in Table 14.16 (in PDF or PS) of (1976AJ04). See also (1976BO1Q: E_d = 1.6 to 3.0 MeV). For total cross-section measurements at E_d = 1.55 and 2.89 GeV/c see (1978JA16). See also (1979DE1P).

Polarization measurements to E_d = 51 MeV are displayed in Table 14.17 (in PDF or PS) of (1976AJ04). Recent work has been carried out at E_d = 12.6 MeV (1976ZA1B; d₀; VAP), E_d-bar = 29.5 MeV (1977PE07; d₀; VAP, TAP) and 52 MeV (1980MA10, 1976BE1U; to ¹²C*(0, 4.4, 9.6)). The (d, np) processes are discussed in reaction 50 of ¹²C in (1980AJ01), reaction 36 in ¹³C and reaction 19 in ¹³N. See also (1976GE20). See also (1975BO58, 1977FR12, 1978HA1Q; theor.).

16. (a) ¹²C(d, t)¹¹C Q_m = -12.464 E_b = 10.27240
(b) ¹²C(d, ³He)¹¹B Q_m = -10.4634

At E_d-bar = 29 MeV, polarizations to the ground states of ¹¹B and ¹¹C have been studied by (1978CO13). See also (1976AJ04).

17. ¹²C(d, α)¹⁰B Q_m = -1.3408 E_b = 10.27240

Reported resonances are displayed in Table 14.14 (in PDF or PS). Listings of measurements of the yields of α-groups to E_d-bar to 29.5 MeV are given in Tables 14.16 (in PDF or PS) (1976AJ04) and 14.11 (in PDF or PS) (1970AJ04).

The major interest in this reaction has been the study of the yield of the α₂ group to the J^π = 0⁺, isospin "forbidden" T = 1 state. In particular, the work of (1972SM07, 1971RI15) has shown that while the α₀, α₁ and α₃ yields show only weak fluctuations, the α₂ "forbidden" yield shows narrow resonances which implies that the source of the isospin mixing (at least in the region which they, and the subsequent work of (1974JO01) studied: E_d = 7.2 to 16 MeV) is due to states in the ¹⁴N compound nucleus. The ratio of the σ_t for the α₂ group compared to the σ_t for the "allowed" groups is ≈ 1%, an order of magnitude greater than predicted by direct or multistep processes (1972SM07). Partial wave analyses lead to the resonance parameters shown in Table 14.14 (in PDF or PS) (1972SM07, 1974JO01). See also (1970AJ04).

Polarization measurements are reported for the α₀ → α₄ groups at E_d-bar = 11 to 14 MeV (1976PE08) and 20.7 and 29 MeV (1977CO17). See also (1976KU1D), (1974LO1B) and (1977TO1E, 1978IZ02, 1979SE04; theor.).

18. (a) ¹²C(d, ⁶Li)⁸Be Q_m = -5.893 E_b = 10.27240
(b) ¹²C(d, ⁷Li)⁷Be Q_m = -17.542

Vector analyzing power measurements have been carried out at E_d-bar = 16 MeV for the group to ⁸Be_g.s. (1976JA1G). See also (1976JA1H) and ⁷Be and ⁸Be in (1979AJ01).

19. ¹²C(t, n)¹⁴N Q_m = 4.01507

Angular distributions have been measured at E_t = 1.12 to 1.68 MeV (1971MA46: n₀, n₁, n₂) and at 8 MeV (1972CO01: to ¹⁴N states with E_x < 8.7 MeV).

20. ¹²C(³He, p)¹⁴N Q_m = 4.7788

Observed proton groups are displayed in Table 14.15 (in PDF or PS). Angular distributions have been measured for E(³He) to 25.3 MeV: see (1970AJ04, 1976AJ04).

Extensive studies of p'γ and p'p correlations (the latter from ¹²C(³He, p')¹⁴N*(p)¹³C_g.s.) have led to the confirmation and determination of J^π of many of the unbound states: see Tables 14.15 (in PDF or PS) and 14.11 (in PDF or PS): see (1970AJ04, 1976AJ04) for a fuller discussion and a listing of the relevant references. Recently (1977HE04: E(³He) = 11 to 20 MeV) have studied p'γ angular correlations involving ¹⁴N*(3.95, 5.10, 5.69, 6.21, 7.03). (1978MO27) find |g| = 0.66 ± 0.04 for ¹⁴N*(5.11): τ_m for ¹⁴N*(5.11, 5.83) are displayed in Table 14.12 (in PDF or PS). See also (1978MO1N). See also ¹⁵O, (1966YO1A, 1979HAYZ), (1974LO1B) and (1976EP1A; astrophys.).

21. ¹²C(α, d)¹⁴N Q_m = -13.57434

Angular distributions of deuterons corresponding to T = 0 states in ¹⁴N have been measured at E_α = 42 MeV: see Table 14.19 (in PDF or PS) in (1976AJ04), and (1970AJ04) for a listing of the references. At E_α = 55 MeV, d₀ and d₁ angular distributions have been studied by (1976VA07). The deuteron spectrum is dominated by very strong groups corresponding to the (d_5/2)², J^π = 5⁺ state at 8.96 MeV, and to a state at 15.1 MeV: see (1976AJ04). See also (1976BU21).

22. ¹²C(⁶Li, α)¹⁴N Q_m = 8.7989

At E(⁶Li) = 20 MeV, α groups corresponding to most of the T = 0 states with E_x < 12.7 MeV are reported: see Table 14.19 (in PDF or PS) in (1976AJ04). The spectrum is dominated by the α-group corresponding to the 5⁺ state at 9.0 MeV (1968ME10). Angular distributions have also been measured for E(⁶Li) = 2 to 33 MeV [see (1970AJ04, 1976AJ04)] and at E(⁶Li) = 10.5 to 13.75 and 20 MeV (1975SO1E, 1978SO01: α₀, α₁, α₂) and E(pol. ⁶Li) = 20 MeV (1978MA13, 1979MA1T: analyzing power, all known T = 0 states with E_x < 10.9 MeV). For the yield of the isospin "forbidden" group, α₁, see ¹⁸F in (1978AJ03, 1983AJ01). See also (1978AR01) and (1977WE08, 1978ME20; theor.).

23. ¹²C(⁹Be, ⁷Li)¹⁴N Q_m = -6.424

See (1976AJ04).

24. ¹²C(¹¹B, ⁹Be)¹⁴N Q_m = -5.544

At E(¹¹B) = 114 MeV the spectrum is dominated by groups to the 5⁺ state at E_x = 8.96 MeV and to one or more of the states at 12.8 MeV, presumably the 4⁺ one (1974AN36, 1975PO10). See also (1976AJ04).

25. ¹²C(¹²C, ¹⁰B)¹⁴N Q_m = -14.915

This reaction has been studied at E(¹²C) = 114 MeV: the spectrum is dominated by ¹⁴N*(8.96)[J^π = 5⁺] but there is substantial population also of ¹⁴N*(5.83) [3^-] and of a state at E_x = 11.2 MeV (1974AN36). Angular distributions are reported at E(¹²C) = 58 to 64.5 MeV (1979CL06) and at 93.8 MeV (1979FU04).

26. ¹²C(¹⁸F, ¹⁶O)¹⁴N Q_m = 2.746

See (1976AJ04).

27. ¹²C(²⁰Ne, ¹⁸F)¹⁴N Q_m = -10.779

See (1979MEZX).

28. (a) ¹³C(p, γ)¹⁴N Q_m = 7.55063
(b) ¹³C(p, p'γ)¹³C E_b = 7.55063

Observed resonances are displayed in Table 14.16 (in PDF or PS). The decay schemes of various levels of ¹⁴N, as derived from the γ-spectra in this and other reactions, are exhibited in Table 14.11 (in PDF or PS). For τ_m see Table 14.12 (in PDF or PS) and (1977BI07, 1980AN1E).

The low-energy capture cross section yields an extrapolated S-factor at E_p = 25 keV (c.m.), S₀ = 6.0 ± 0.8 keV · b (1960HE14). See also (1970AJ04). The capture cross section rises from (7.7 ± 1.8) × 10^-10 b at E_p = 100 keV to (9.8 ± 1.2) × 10^-9 b at E_p = 140 keV (1961HE02).

Following is a summary of the reasons for the assignments of J^π; T to some of the lower resonances displayed in Table 14.16 (in PDF or PS): for a fuller discussion and complete references see (1970AJ04, 1976AJ04) and see Table 14.11 (in PDF or PS). ¹⁴N*(7.97): angular distribution of the γ-rays is consistent with J^π = 2^-. ¹⁴N*(8.06): width of resonance, isotropy of γ-rays show l_p = 0: J^π = 1^- from ¹³C(p, p); E1 transition to g.s. is uninhibited, e.g., T = 1 [but 1.4% 8.06 → 2.3 transition [E_x = 2312.6 ± 0.3 keV] shows T = 0 admixture: α² = 0.046]. The strong transition 8.06 → 5.69 [3.5%] permits either E1 or M1, ΔT = 1. Since 5.69 → 2.31 is seen ¹⁴N*(5.69) cannot have J^π = 0⁺, and 2⁺ is excluded by the strength of the 8.62 → 5.69 transition. It is then J^π = 1^-; T = 0 [the isospin mixing α² = 0.09]; E_x = 5690.5 ± 1.5 keV. ¹⁴N*(8.49, 8.96, 9.12) correspond to anomalies in the cross section. The nature of their γ-decays [see Table 14.11 (in PDF or PS)] and the angular distribution leads to J^π; T = 4^-; 0, 5⁺; 0, 3⁺; 0, respectively [see (1978KE01) for a recent study of ¹⁴N*(9.13)].

¹⁴N*(8.62) [J^π = 0⁺ from ¹³C(p, p)] shows strong transitions to ¹⁴N*(0, 3.95, 5.69): T = 1. The strength of the 8.62 → 3.95 decay shows it is dipole and therefore J = 1 for ¹⁴N*(3.95) [E_x = 3947.6 ± 0.4 keV]. The strength of the transition 8.62 → 6.21 and the angular correlation 8.62 → 6.21 → g.s. is consistent with J^π = 1⁺, T = 0 for ¹⁴N*(6.20) [E_x = 6203.7 ± 0.6 keV]. ¹⁴N*(8.79) [J^π = 0^- from ¹³C(p, p)] has a large Γ_γ consistent with E1 and T = 1. ¹⁴N*(9.17): angular correlation and angular distribution measurements indicate J^π = 2⁺ for that state, 3^- for ¹⁴N*(6.44) [see, however, Table 14.10 (in PDF or PS)] and J = 2 for ¹⁴N*(7.03).

The angular distribution of the γ-rays from 10.23 → 2.31 is consistent with J^π = 1⁺ for ¹⁴N*(10.23): T = 0 from M²(M1) [see, however, Table 14.10 (in PDF or PS)]. The γ₀ angular distribution is consistent with J = 2 for ¹⁴N*(10.43): the similar decay characteristics of this state and of ¹⁴N*(9.17) suggest that they are both J^π = 2⁺, T = 1.

Below E_p = 5.5 MeV only γ₀ can be observed in the capture radiation. (1971RI13) have observed a number of resonances in the γ₀ yield and in the yield of the ground state γ-rays from ¹³C*(3.09, 3.68, 3.85): these are shown in Table 14.16 (in PDF or PS) in the range E_p = 3.7 to 6.6 MeV [see reaction 25 in (1970AJ04) for the earlier work]. Angular distributions and measurements of Γ_γ₀ lead to the J^π values shown. Above E_p = 7 MeV the γ₀ yield shows broad structure and the giant dipole resonance at E_x = 22.5 and 23.0 MeV (1971RI13). Measurements by (1975PA18) of the γ₀ and γ₁ 90° yields for E_x = 23 to 33 MeV find that the T = 2 resonances reported by (1971RI13) at E_x = 23.7 and 24.2 MeV do not exist and that there is no evidence for the T = 2 GDR between E_x = 25 and 29 MeV (1975PA18). The 90° yields of γ-rays to T = 0 states (4.9 < E_x < 5.9 MeV) and to T = 1 states (8.0 < E_x < 9.5 MeV) have been measured from E_x = 23 and 26 MeV, respectively, to E_x = 33 MeV (1975PA18). A recent study of the 90° yield of γ₀ and γ₁ [and of analyzing powers] has been reported for E_p-bar = 6.25 to 17.0 MeV by (1980TU01). The γ₀ results are in good agreement with those of (1974BA37) in the inverse reaction [¹⁴N(γ, p)¹³C]. Broad structures are observed at E_p ≈ 8, 13, 14, 15 and 16.5 MeV. The γ₁ results indicate that the T = 0 strength is spread out fairly uniformly between E_x = 13 and 23 MeV (1980TU01). At E_p = 25 MeV strong transitions are observed to two groups of states centered near E_x = 5.8 and 8.9 MeV (1980MA1E).

See also (1966YO1A, 1976KR1A, 1979TR1G) and (1975ZI1A, 1976BR1H; astrophys.).

29. ¹³C(p, p)¹³C E_b = 7.55063

The elastic scattering has been studied for E_p = 0.14 MeV to 11 MeV: see (1970AJ04, 1976AJ04). For observed resonances see Table 14.16 (in PDF or PS); for angular distributions see ¹³C. The yields of p₀ at eight angles (and the analyzing power) have been measured for E_p-bar = 9.1 to 18.4 MeV. A phase shift analysis implies the existence of resonances with J^π = 1^-, 2^- and 3⁺ in the vicinity of E_p ≈ 15 MeV. The 1^- and 2^- resonances have widths of ≈ 3 - 4 MeV and have a total Γ_p/Γ value of 0.1. The correlation between these resonances and the GDR is not clear. There is no indication of the T = 2 states previously reported in reaction 30 (1978WE13). For other polarization measurements see (1976AJ04) and (1976TR1C). See also (1978DW1A; astrophys.).

30. ¹³C(p, n)¹³N Q_m = -3.0030 E_b = 7.55063

The yield of neutrons has been measured from threshold to E_p = 13.7 MeV: see (1970AJ04). Observed resonances are displayed in Table 14.17 (in PDF or PS). The ratio of the reaction cross section at E_p = 22.8 MeV to the n₀ yield is 1.06 ± 0.07: thus there is little competition of γ-rays from excited states of ¹³N with neutron emission making this a convenient fast neutron calibration source (1975LI11). The 0° polarization transfer coefficients have been measured for E_p-bar = 7.9 to 14.6 MeV (1976LI08). For other polarization measurements see (1965WA02; n₀; E_p = 6.9 to 12.3 MeV) and (1979CLZS; 6 MeV). See also (1979BYZZ), (1974LO1B, 1976WA1B, 1979BY1B) and ¹³N.

31. ¹³C(p, d)¹²C Q_m = -2.7218 E_b = 7.55063

Analyzing power measurements for ¹²C*(0, 12.71, 15.11, 16.11) have been measured at E_p-bar = 65 MeV (1979HO1H) and those for ¹²C*(0, 4.4) are reported at E_p-bar = 200 MeV (1979CA1A). See also (1976AJ04), ¹²C in (1980AJ01) and (1980MC1C, 1980WH1A).

32. (a) ¹³C(p, t)¹¹C Q_m = -15.186 E_b = 7.55063
(b) ¹³C(p, ³He)¹¹B Q_m = -13.1851

At E_p = 49.6 MeV polarization measurements have been carried out for the tritons and ³He ions to the mirror groups ¹¹B*(0, 2.12, 4.45, 5.02, 6.74, 12.91) and ¹¹C*(0, 2.00, 4.32, 4.80, 6.48, 12.50) (1974MA12). See also (1976AJ04) and ¹¹B, ¹¹C in (1980AJ01).

33. ¹³C(p, α)¹⁰B Q_m = -4.0626 E_b = 7.55063

Excitation functions have been measured from E_p = 5.5 (α₀), 6.0 (α₁), 7.0 (α₂), 8.0 (α₃), 10 (α₄), 11 (α to ¹⁰B*(5.11)) to 18 MeV. Total cross sections have also been obtained for the production of ⁶Li, ⁹Be and ¹⁰B: the latter shows a great deal of structure. The consequences for astrophysical problems are discussed by (1975OB01). The analyzing power for the α₀ group has been measured at E_p-bar = 65 MeV by (1980KA03). See also ¹⁰B in (1979AJ01).

34. ¹³C(d, n)¹⁴N Q_m = 5.3260

Observed neutron groups are displayed in Table 14.18 (in PDF or PS). Angular distributions have been reported at many energies up to E_d = 12 MeV: see (1970AJ04) and Table 14.18 (in PDF or PS). Comparisons of relative spectroscopic factors obtained in this reaction and in reaction 35 are shown in Table 14.23 (in PDF or PS) of (1976AJ04): it appears that S_rel for ¹⁴N*(2.31) [T = 1] is smaller in this reaction than in the (³He, d) reaction although simple DWBA calculations would suggest that the factors would be the same in both proton pickup reactions. The τ · T terms appear to be energy dependent: see Table 14.23 (in PDF or PS) (1976AJ04). See also ¹⁵N and (1976FOZW).

35. ¹³C(³He, d)¹⁴N Q_m = 2.0571

Angular distributions have been studied at E(³He) = 13 to 17 MeV [see (1976AJ04) and Table 14.18 (in PDF or PS)]. At E(³He) = 13 MeV the angular distributions of deuterons and singlet deuterons to ¹⁴N*(0, 2.31, 3.95) have been investigated by (1976JA14): the relative spectroscopic factors for these three states are 1.0, 1.50, 0.43 for deuterons and 1.0, 1.57, 0.41 for singlet deuterons. Spectroscopic factors for these and other states of ¹⁴N observed in this reaction and in reaction 34 are displayed in Table 14.23 (in PDF or PS) of (1976AJ04). At E(³He) = 43.6 MeV ¹⁴N*(8.91, 9.51) are strongly populated while ¹⁴N*(8.49, 9.13, 9.39) are weakly excited. The d_5/2 transfer to T = 0 states is concentrated in the transitions to ¹⁴N*(5.11, 5.83) (1980HA1E). See also (1979MA2K; theor.).

36. ¹³C(α, t)¹⁴N Q_m = -12.2634

Angular distributions have been measured at E_α = 27 MeV for the α groups to ¹⁴N*(0, 2.31, 3.95, 4.92, 5.11). See also (1976AJ04), (1976LE1K) and (1978ZE03, 1980ZE05; theor.).

37. ¹³C(⁷Li, ⁶He)¹⁴N Q_m = -2.424

At E(⁷Li) = 34 MeV, angular distributions have been obtained for the transitions to ¹⁴N*(0, 2.31, 3.95) (1973SC26).

38. ¹³C(¹¹B, ¹⁰Be)¹⁴N Q_m = -3.678

See (1976AJ04).

39. ¹⁴C(β^-)¹⁴N Q_m = 0.15648

See ¹⁴C.

40. ¹⁴C(p, n)¹⁴N Q_m = -0.6259

Angular distributions have been obtained for the n₀, n₁ and n₂ groups in the range E_p = 6 to 14 MeV [see (1976AJ04)] and at E_p = 2.45 MeV (1977NI03; n₀) and 35 MeV (1979DO14; n₀, n₂). DWBA analysis of the latter results favors the inclusion of an isovector tensor interaction in the transition to ¹⁴N_g.s. (1979DO14). See also ¹⁵N.

41. ¹⁴C(³He, t)¹⁴N Q_m = 0.1379

At E(³He) = 44.8 MeV, triton groups are observed corresponding to all known levels of ¹⁴N with E_x < 7.1 MeV. Triton groups were also seen to unresolved states with E_x = 8.0 → 9.5 MeV, to ¹⁴N*(10.43) and to excited states with E_x = 12.49 ± 0.04, 12.83 ± 0.05 and 13.70 ± 0.04 MeV. Angular distributions were obtained for nine of the triton groups and analyzed using a local two-body interaction with an arbitrary spin-isospin exchange mixture. Dominant L = 0 transitions are found to ¹⁴N*(2.31, 3.95, 13.7), L = 1 to ¹⁴N*(5.11), L = 2 to ¹⁴N*(0, 7.03, 10.43) and L = 3 to ¹⁴N*(5.83) (1969BA06). See also reaction 50.

42. (a) ¹⁴C(⁶Li, ⁶He)¹⁴N Q_m = -3.350
(b) ¹⁴C(¹⁴C, ¹⁴B)¹⁴N Q_m = -20.47
(c) ¹⁴C(¹⁸O, ¹⁸N)¹⁴N Q_m = -13.90

Angular distributions have been studied at E(⁶Li) = 62 MeV for the transitions to ¹⁴N*(0, 3.95, 6.20, 7.03): the L = 0 transition to ¹⁴N*(3.95) carries at least 90% of the GT strength (1976GO25). For reactions (b) and (c) see (1980NA14).

43. (a) ¹⁴N(γ, n)¹³N Q_m = -10.554
(b) ¹⁴N(γ, p)¹³C Q_m = -7.55063
(c) ¹⁴N(γ, d)¹²C Q_m = -10.27240
(d) ¹⁴N(γ, 2n)¹²N Q_m = -30.617

The total absorption over the range E_γ = 9 to 31 MeV is dominated by a single peak at 22.5 MeV [estimated σ ≈ 29 mb, Γ ≈ 2 - 3 MeV] and appreciable strength extending beyond 30 MeV. The cross section cannot be accounted for solely by the (γ, n) and (γ, p₀) processes: particle unstable excited states of ¹³C, ¹³N are involved (1969BE92). The combined (γ, n) and (γ, pn) cross section begins to rise rapidly above 18 MeV, reaches its maximum value of 15 mb at 23.3 MeV and exhibits structure at about 19, 20.5 and 26 MeV. The main peak (Γ ≈ 3.5 MeV: see (1970AJ04)) at 23.3 MeV appears to be split into two absorption levels (1970BE54, 1975BE60, 1975BE1F, 1976BE1H: monoenergetic photons) and (1980JU02). Maxima reported in other experiments and "breaks" in the (γ, n) activation curve are listed in (1970AJ04). Most of the photon absorption in the giant resonance region forms J^π = 2^- states in ¹⁴N which decay by d-wave neutron emission to ¹³N_g.s.. Some evidence is found for the existence of J^π = 0^- strength at the peak of the giant resonance. Some evidence exists for a small amount of isospin T = 0 mixing near 22.5 MeV (1980JU02).

The (γ, p₀) and (γ, p₂) cross sections and angular distributions have been measured in the giant resonance region by (1972CA34, 1974BA37). The authors infer that the giant dipole states [(p_3/2)^-1(2s1d)] which decay by p₀ emission to ¹³C*(3.68) carry ≈ 90% of the E1 strength and do not contribute substantially to the (γ, p₀) process which is populated by (p_1/2)^-1(2s1d) giant dipole states. Above E_γ = 22 MeV d-wave emission from 2^- states appears to dominate the (γ, p₀) cross section (1972CA34, 1974BA37). See also reaction 30.

For reaction (c) see (1977TA1B); for reaction (d) see (1979WI1A). For spallation reactions see (1970AJ04) and (1976TU05, 1978DI1A). See also (1974BU1A, 1977DA1B) and (1979ME1E, 1980ME12; theor.).

44. ¹⁴N(γ, γ)¹⁴N

See (1976AJ04) and Table 14.19 (in PDF or PS).

45. (a) ¹⁴N(e, e')¹⁴N
(b) ¹⁴N(e, ep)¹³C Q_m = -7.55063

The r.m.s. radius of ¹⁴N is 2.54 ± 0.02 fm: see (1976AJ04). Form factors have been determined at E_e = 60.7 to 122.0 MeV for ¹⁴N*(2.31, 3.95, 4.92, 5.11, 5.69, 5.83): the reduced transition probabilities for these states, in single-particle units, are, respectively, 0.065 ± 0.020, 1.70 ± 0.14, (1.1 ± 0.5) × 10^-7, 4.1 ± 1.0, (3.8 ± 2.1) × 10^-8 and 6.1 ± 1.3 (1974EN01). E.K. Warburton (private communication) calculates 8.7 ± 0.9 fsec for the τ_m of ¹⁴N*(3.95), on the basis of (1974EN01), the branching ratios of Table 14.11 (in PDF or PS), and the δ(E2/M1) of (1967OL02). Inelastic scattering (at θ = 180°) gives evidence for the excitation of states with E_x = 8.91 to 16.11 MeV: see Table 14.19 (in PDF or PS). See also Table 14.11 (in PDF or PS).

See also (1977FR1M, 1978VO12), (1977RI1H) and (1976BH1B, 1978FU13, 1979DO1P, 1979DO17, 1979KI1K, 1980ER01; theor.). For reaction (b) see (1978DE32).

46. ¹⁴N(n, n')¹⁴N*

Angular distributions of elastically and inelastically scattered neutrons are displayed in Table 14.23 (in PDF or PS) of (1970AJ04). See also (1975BE1Y, 1978BE2B). Observed γ-rays are shown in Table 14.25 (in PDF or PS) of (1976AJ04). See also (1979SO1B; applied).

47. (a) ¹⁴N(p, p')¹⁴N*
(b) ¹⁴N(p, 2p)¹³C Q_m = -7.55063
(c) ¹⁴N(p, pd)¹²C Q_m = -10.27240

Angular distributions of elastically and inelastically scattered protons have been studied at a number of energies up to E_p = 155 MeV: see Tables 14.23 (in PDF or PS) in (1970AJ04) and 14.26 (in PDF or PS) in (1976AJ04) and (1977SA1B; p₀; E_p = 5.85 MeV), (1979AO02; p₀, p₁; 21 MeV; pol.), (1980FO05; p₀, p₁, p₂ and see Table 14.20 (in PDF or PS); 29.8, 36.6 and 40.0 MeV), (1980FA07; p₀; 35.2 MeV), (1980CO05; p₀, p₁, p₂; 122 MeV) and (1980MO01; p₀; 144 MeV).

(1980FO05) have analyzed angular distributions to ¹⁴N*(2.31) with a microscopic model DWA which included contributions from the knock-on exchange amplitude and from central, tensor and spin-orbit forces. The first were fairly satisfactory. The extracted strengths of the tensor force were 20 - 75% larger than estimates based on the one-pion-exchange potential (1980FO05). See also (1976AJ04).

Observed inelastic groups are exhibited in Table 14.20 (in PDF or PS). At E_p = 800 MeV, the spectra are dominated by the groups to ¹⁴N*(9.17, 10.43) [J^π = 2⁺] (1979MO1E; prelim.).

For reaction (b) see (1976AJ04). For reaction (c) see (1970AJ04). See also (1977BA85), (1979RA1C; astrophys.), (1976DO12, 1977GA22, 1978GO1L, 1978MA34, 1979KI10, 1979MA20; theor.) and ¹⁵O.

48. ¹⁴N(d, d')¹⁴N*

Angular distributions of elastically and inelastically scattered deuterons have been studied for E_d = 52 MeV: see Table 14.23 (in PDF or PS) in (1970AJ04), (1976AJ04), (1980KR01; d₀; E_d-bar = 10 MeV), and (1976AO01, 1979AO01; d₀, d₁, d₂; E_d = 10.0, 11.7, 14.8, 17.9 MeV). Inelastic groups are displayed in Table 14.20 (in PDF or PS). The deuteron group to the 0⁺, T = 1 state ¹⁴N*(2.31) is isospin forbidden: its cross section is 1 - 2 orders of magnitude less than that to ¹⁴N*(3.95) [J^π; T = 1⁺; 0]. It is summarized for E_d = 6 to 20 MeV by (1979AO01) who find that the observed isospin violation is well accounted for by a direct multistep reaction mechanism which assumes that there is isospin mixing in the intermediate channels. See also (1976AJ04), ¹⁶O in (1977AJ02, 1982AJ01) and (1977IZ01, 1977IZ1B, 1978MA34; theor.).

49. ¹⁴N(t, t)¹⁴N

See (1976AJ04).

50. ¹⁴N(³He, ³He')¹⁴N*

Angular distributions of elastically and inelastically scattered ³He ions have been measured at E(³He) up to 44.6 MeV: see Table 14.23 (in PDF or PS) in (1970AJ04) and (1976AJ04).

At E(³He) = 44.6 MeV, twelve ³He groups are reported corresponding to states in ¹⁴N: see Table 14.20 (in PDF or PS) (1969BA06). The angular distributions were analyzed using a local two-body interaction with an arbitrary spin-isospin exchange mixture. A comparison of the cross sections of the reactions ¹⁴N(³He, t)¹⁴O_g.s., ¹⁴N(³He, ³He')¹⁴N*(2.31) and ¹⁴C(³He, t)¹⁴N(0) [which all correspond to transitions between identical initial and final states] shows that they are roughly equal, as would be expected from charge independence, once detailed-balance, isospin coupling and phase-space corrections have been applied (1969BA06).

51. (a) ¹⁴N(α, α')¹⁴N*
(b) ¹⁴N(α, ⁸Be)¹⁰B Q_m = -11.7051

Angular distributions of elastically and inelastically scattered α-particles have been measured for E_α = 7.6 to 104 MeV: see Table 14.23 (in PDF or PS) in (1970AJ04) and (1976AJ04), (1974CH1T, 1976CH24; α₁; E_α = 7.6 to 16.9 MeV), (1977EN01; α₀; 19.8 to 23.1 MeV) and (1976FE12; α₀, α_2→4, α₅₊₆, α₇₊₈, α₉, α₁₀; 23.7 MeV). Table 14.20 (in PDF or PS) displays the observed α-groups. Generally the intensity of the α₁ group is weak: see (1976CH24) and ¹⁸F in (1978AJ03, 1983AJ01). See also (1976YO02). (1976WO11) find S_α = 0.75 for ¹⁴N_g.s.. See also (1977KN1E), (1976HA1Q, 1977MA2E, 1979KN1F), (1979RA1C; astrophys.) and (1977DM1A; theor.).

52. (a) ¹⁴N(⁶Li, ⁶Li)¹⁴N
(b) ¹⁴N(⁷Li, ⁷Li)¹⁴N

Elastic angular distributions have been measured at E(⁶Li) = 19.5 MeV (1977KU06) and 32 MeV (1971GR44) and at E(⁷Li) = 36 MeV (1976CO23).

53. ¹⁴N(⁹Be, ⁹Be)¹⁴N

See ⁹Be in (1974AJ01).

54. (a) ¹⁴N(¹⁰B, ¹⁰B)¹⁴N
(b) ¹⁴N(¹¹B, ¹¹B)¹⁴N

Elastic angular distributions (reaction (a)) have been measured at E(¹⁰B) = 100 MeV (1975NA15) and E(¹⁴N) = 73.9 and 93.6 MeV (1977MO1A, 1979MO14). The elastic distributions (reaction (b)) have been studied at E(¹⁴N) = 41, 77 and 113 MeV (1971LI11). For fusion cross sections see (1977HI01, 1978KO1J, 1978WU1C, 1980OR1C). See also (1978TA1B).

55. ¹⁴N(¹²C, ¹²C)¹⁴N

Elastic angular distributions have been measured in the range E(¹⁴N) = 21.3 to 155 MeV: see (1976AJ04). More recently studies are reported at E(¹⁴N) = 37, 47 and 58.3 MeV (1978CO20), 53 MeV (1976ZE04) and 78.8 MeV (1977MO1A, 1979MO14). At E(¹⁴N) = 155 MeV the selective population of certain ¹⁴N states is observed and angular distributions are reported for the transitions to ¹⁴N*(0, 8.96, 12.7) (1975NA11).

For fusion cross section measurements see (1976ST12, 1977SW02, 1979GO09, 1979GO11, 1979KO20, 1980WI09) and (1976AJ04). See also (1978DA1E, 1978HA1F), (1976LE1F, 1978TS04, 1979GO1R, 1979NA1G, 1980TA1B), (1978RO1D; astrophys.) and (1976AM01, 1977BA3E, 1977MA11, 1978AV1A, 1978CU1C, 1978CU1E, 1978CU06, 1978FR1N, 1978HO13, 1978KA14, 1978VA1A, 1979MO1J, 1979NA03, 1980LE11, 1980LO02, 1980VA03; theor.).

56. (a) ¹⁴N(¹³C, ¹³C)¹⁴N
(b) ¹⁴N(¹⁴C, ¹⁴C)¹⁴N

The elastic angular distribution (reaction (a)) has been measured at E(¹⁴N) = 19.3 MeV (1971VO01). For a fusion study see (1980WI09). For reaction (b) see (1976AJ04).

57. ¹⁴N(¹⁴N, ¹⁴N)¹⁴N

Elastic angular distributions have been studied for E(¹⁴N) = 4.99 to 20.22 MeV (1969JA15). For fusion cross section measurements see (1976ST12, 1976SW02). See also (1976AJ04), (1978RO1D; astrophys.) and (1976RU1B, 1978AV1A, 1979HU1B; theor.).

58. ¹⁴N(¹⁶O, ¹⁶O)¹⁴N

Elastic angular distributions have been measured for E(¹⁴N) = 8.08 to 155 MeV: see (1976AJ04). Recent work is reported at E(¹⁴N) = 76.2 MeV (1977MO1A, 1979MO14) and 155 MeV (1977TO02: see also ¹⁶O in (1982AJ01)). For fusion cross section measurements see (1976ST12, 1977SW02, 1977VO08). See also (1976AJ04) and (1978AV1A, 1978VA1A; theor.).

59. ¹⁴N(¹⁹F, ¹⁹F)¹⁴N

The elastic scattering has been studied at E(¹⁴N) = 19.5 MeV (1977KU06).

60. (a) ¹⁴N(²⁴Mg, ²⁴Mg)¹⁴N
(b) ¹⁴N(²⁷Al, ²⁷Al)¹⁴N
(c) ¹⁴N(²⁸Si, ²⁸Si)¹⁴N
(d) ¹⁴N(²⁹Si, ²⁹Si)¹⁴N

For reactions (a, b, c) see (1977TH1G). For reactions (b, c) see (1971KO11: E(¹⁴N) = 65, 84 and 88 MeV). For reaction (c) see (1977EC04: E(¹⁴N) = 27, 30 and 33 MeV). For reaction (d) see (1978PE13: E(¹⁴N) = 39 MeV). See also (1977SC1G, 1980TA1B) and (1979KA27; theor.).

61. (a) ¹⁴N(³⁹K, ³⁹K)¹⁴N
(b) ¹⁴N(⁴⁰Ca, ⁴⁰Ca)¹⁴N
(c) ¹⁴N(⁴⁸Ca, ⁴⁸Ca)¹⁴N

For reaction (a) see (1978BA26; theor.). For reaction (b) see (1978BU10), (1978HO1C) and (1979SA27; theor.). For reaction (c) see (1978HO1C).

62. ¹⁵N(γ, n)¹⁴N Q_m = -10.8334

Cross sections (integrated to 35 MeV) have been measured for the transitions to ¹⁴N*(2.31, 3.95, 5.11 + 5.83, 7.03) (1976PA22). See also ¹⁵N.

63. ¹⁵N(p, d)¹⁴N Q_m = -8.6087

Angular distributions have been obtained for the deuterons corresponding to ¹⁴N*(0 → 8.06, 8.62, 8.91, 8.96 + 8.98, 9.17 → 10.43, 10.81, 11.05, 11.24 + 11.29, 11.36 → 11.66, 11.75, 11.95, 12.20, 12.50, 12.61, 12.79 + 12.82, 13.17 + 13.24, 13.71 + 13.72) (1969SN04: E_p = 39.8 MeV). Spectroscopic factors were extracted by DWBA analysis of the l_n = 1 pickup angular distributions (1969SN04). See also (1976AJ04).

64. ¹⁵N(³He, α)¹⁴N Q_m = 9.7445

Observed states in ¹⁴N are displayed in Table 14.28 (in PDF or PS) of (1976AJ04) together with the derived spectroscopic factors.

65. ¹⁵N(¹³C, ¹⁴C)¹⁴N Q_m = -2.6568

At E(¹⁵N) = 30, 32 and 45 MeV the angular distributions involving ¹⁴N*(0, 2.31) have been studied: they are symmetric about 90° for the transition to the T = 1 analog state ¹⁴N*(2.31) (1975GA17, 1976GA37).

66. ¹⁶O(π^-, 2n)¹⁴N Q_m = 155.824

At E_π^- = 230 MeV, γ-rays from the decay of ¹⁴N*(2.31, 3.95, 5.11, 5.83) are observed (1974LI15).

67. (a) ¹⁶O(γ, d)¹⁴N Q_m = -20.7363
(b) ¹⁶O(p, pd)¹⁴N Q_m = -20.7363

For reaction (a) see (1979WIZW) and ¹⁶O in (1982AJ01). At E_p = 75 MeV, angular distributions to ¹⁴N*(0, 3.95) have been studied by (1977GR04); ¹⁴N*(2.31) is also populated. See also (1976GO1E).

68. ¹⁶O(p, ³He)¹⁴N Q_m = -15.2428

Angular distributions have been measured in the range E_p = 27 to 54.1 MeV: see (1976AJ04) and at E_p = 27.0 to 30.7 MeV (1978GO04; to ¹⁴N*(2.31)). A number of comparisons have been made of the ratio of (p, ³He) to the T = 1 state at 2.31 MeV and of (p, t) to the analog ground state of ¹⁴O: see e.g. (1978GO04). See also ¹⁷F in (1982AJ01) and (1976DA1K).

69. ¹⁶O(d, α)¹⁴N Q_m = 3.1104

Angular distributions have been measured at many energies up to E_d = 40 MeV: see Table 14.25 in (in PDF or PS) (1970AJ04), (1976AJ04) and (1973CA30; α₀; 0.98 → 1.97 MeV), (1976LU1A; α₀, α₂; 16 MeV) and (1976VA07: α to ¹⁴N*(0, 3.95, 7.03, 11.04; 40 MeV). Analysis with a one-step ZRDWBA is reported by (1976VA07) And S values are derived: ¹⁴N*(11.04) probably has J^π = 3⁺.

The yield of the isospin forbidden α₁ group [to ¹⁴N*(2.31)] has been studied for E_d = 2 to 15 MeV by (1969JO09, 1973JO13): the intensity of the isospin group is strongly dependent on E_d and on the angle of observation. The α₁ reaction appears to proceed almost exclusively by a compound nuclear process and its study leads to the determination of a large number of ¹⁸F states: the average isospin impurity in ¹⁸F for 10 ≤ E_x ≤ 20 MeV is 3 - 10% (1973JO13). At E_d = 50 MeV, the intensity of ¹⁴N*(2.31) is 0.1 - 0.2% that of ¹⁴N_g.s. (1975FA06). See also ¹⁸F in (1978AJ03, 1983AJ01) and (1976PE08, 1978RI05).

Measurements on the absolute cross sections of this reaction [E_d = 3.6 to 5.3 MeV] and its inverse [ ¹⁴N(α, d)¹⁶O] are consistent with the principle of detailed balance. An upper limit of 0.2% is assigned to the time-reversal non-invariant part of the reaction amplitudes (1971TH03). See also (1978HI1E, 1978PI15; applications).

70. ¹⁶O(α, ⁶Li)¹⁴N Q_m = -19.2628

At E_α = 42 MeV the transitions involving (¹⁴N_g.s. and ⁶Li*(0, 3.56)), (¹⁴N*(2.31) + ⁶Li_g.s.) and (¹⁴N*(3.95) + ⁶Li_g.s.) have been studied by (1972RU03).

71. ¹⁶O(¹⁰B, 3α)¹⁴N Q_m = -2.8236

See (1978BE1G).

72. ¹⁶O(¹¹B, ¹³C)¹⁴N Q_m = -2.0576

See (1976AJ04).

73. ¹⁶O(¹⁶O, ¹⁸F)¹⁴N Q_m = -13.2100

See (1974RO04).

74. ¹⁷O(p, α)¹⁴N Q_m = 1.191

See (1978SE08) and ¹⁸F in (1978AJ03, 1983AJ01).

75. ¹⁹F(d, ⁷Li)¹⁴N Q_m = -6.1232

See (1967DE03).