The photon spectrum from stopped pions is dominated by peaks corresponding to <strong>14</strong> C*(6.7+ 6.9+7.0[u], 8.32, 10.7) and branching ratios have been obtained for these and the g.s. transition. That to <strong>14</strong> C*(6.7+6.9+7.0) is (6.22±0.40)% (absolute branching ratio per stopped pion) (86PE05). Fortheearlierworksee(81AJ01). See also the “General” section. 33. <strong>14</strong> N(n, p) <strong>14</strong> C Q m =0.6259 The p 0 angular distribution has been measured at E n = <strong>14</strong> MeV: see (81AJ01). At E n =60 MeV the stongest transitions are to <strong>14</strong> C*(7.0 +8.3, 11.3, 15.4) and to the giant resonanace peak, centered at ≈ 20.4 MeV, and angular distributions have been studied to these groups: see (86AJ01). For cross sections <strong>of</strong> astrophysical interest see 15 N. A study <strong>of</strong> P-odd and left-right asymmetries with polarized thermal neutrons is reported by (88AN19). See also (86BO1K, 88EL1C; applied). 34. <strong>14</strong> N(d, 2p) <strong>14</strong> C Q m = −1.5987 Angular distributions have been measured at E ⃗d =70MeVto <strong>14</strong> C*(7.0[u], 8.3). The ground state is very weakly populated (86MO27). See also (88HE1I). 35. <strong>14</strong> N(t, 3 He) <strong>14</strong> C Q m = −0.13788 At E t =33.4 MeV <strong>14</strong> C*(0, 6.09, 6.73, 7.34, 8.32) are populated (88CL04). 36. <strong>14</strong> N( 7 Li, 7 Be) <strong>14</strong> C Q m = −1.018 See (86GO1B; prelim.; E( <strong>14</strong> N) = 150 MeV). 37. 15 N(γ, p) <strong>14</strong> C Q m = −10.2074 See (81AJ01), 15 Nand(88GOZM; theor.). 38. 15 N(d, 3 He) <strong>14</strong> C Q m = −4.7139 The parameters <strong>of</strong> <strong>14</strong> C states observed in this reaction are displayed in Table <strong>14</strong>.9 <strong>of</strong> (76AJ04). 39. 16 O( 6 Li, 8 B) <strong>14</strong> C Q m = −16.592 At E( 6 Li) = 93 MeV <strong>14</strong> C*(0, 7.01, 8.32, 10.45) are populated, the first two <strong>of</strong> these strongly: see (81AJ01). 26
<strong>14</strong> N (Figs. 3 and 5) GENERAL (See also (86AJ01). <strong>Nuclear</strong> models: (85KW02, 86ZE1A, 87KI1C, 88WO04, 89TA01, 89WO1E, 90HA07, 90VA01) Special states: (85AD1A, 85BA75, 85GO1A, 86ADZT, 86AN07, 86GO29, 87BA2J, 87BL15, 87KI1C, 87SU1G, 88KW1A, 88WRZZ, 89AM01, 89OR02, 89SU1E, 89TA01) Electromagnetic transitions and giant resonances: 87BA2J, 87KI1C, 88YA10, 88WRZZ, 89AM01) (84VA06, 85GO1A, 85GO1B, 86ER1A, Astrophysical questions: (82CA1A, 82WO1A, 85BR1E, 85DW1A, 85PR1D, 86CH1H, 86DO1L, 86HA2D, 86LA1C, 86MA1E, 86SM1A, 86TR1C, 86WO1A, 87AL1B, 87AR1J, 87AR1C, 87AU1A, 87BO1B, 87CU1A, 87DW1A, 87ME1B, 87MU1B, 87PR1A, 87RA1D, 87WA1L, 88BA1H, 88CUZX, 88DU1B, 88DU1G, 88EP1A, 88KR1G, 88WA1I, 89AB1J, 89BO1M, 89CH1X, 89CH1Z, 89DE1J, 89DU1B, 89GU1Q, 89GU28, 89GU1J, 89GU1L, 89HO1F, 89JI1A , 89KA1K, 89KE1D, 89ME1C, 89NO1A, 89PR1D, 89WY1A, 90HA07, 90HO1I, 90RO1E, 90SI1A, 90WE1I) Complex reactions involving <strong>14</strong> N: (84MA1P, 84XI1B, 85BE40, 85KW03, 85PO11, 85RO1F, 85SH1G, 85ST20, 85ST1B, 85WA22, 86AI1A, 86BO1B, 86GR1A, 86GR1B, 86HA1B, 86MA13, 86MA19, 86ME06, 86PL02, 86PO06, 86SA30, 86SH2B, 86SH1F, 86VA23, 86WE1C, 87BA38, 87BE55, 87BE58, 87BO1K, 87BU07, 87FE1A, 87GE1A, 87GO17, 87HI05, 87JA06, 87KO15, 87LY04, 87MU03, 87NA01, 87PA01, 87RI03, 87RO10, 87SH23, 87ST01, 87TE1D, 88AY03, 88CA27, 88GA12, 88HA43, 88KA1L, 88LY1B, 88MI28, 88PAZS, 88POZZ, 88PO1F, 88SA19, 88SH03, 88SI01, 88TE03, 88UT02, 89BA92, 89BR35, 89CA15, 89CEZZ, 89GE11, 89KI13, 89MA45, 89PO06, 89PO07, 89PR02, 89SA10, 89VO19, 89YO02, 89ZHZY, 90BO04, 90DE<strong>14</strong>, 90GL01, 90LE08, 90PA01, 90WE<strong>14</strong>, 90YE02) Applied work: (85GO27, 85KO1V, 86BO1L, 86CO1Q, 86HE1F, 86NO1C, 86PH1A, 86ST1K, 86ZA1A, 87SI1D, 87ZA1D, 88AL1K, 88GO1M, 88IL1A, 88RO1F, 88RO1L, 88ZA1A, 90KO21) Muon and neutrino capture and reactions: 88BU01, 89MU1G, 89NA01, 90CH13, 90GR1G) (85AG1C, 85KO39, 86IS02, 87SU06, 88AL1H, Pion capture and reactions: (83AS01, 84AS05, 85BE1C, 85GI1D, 85KO1Y, 85LA20, 85RO17, 85TU1B, 86AR1F, 86BE1P, 86CE04, 86DY02, 86ER1A, 86GE06, 86KO1G, 86LAZL, 86PE05, 86RA1J, 86RO03, 86SU18, 87AH1A, 87BL15, 87BO1D, 87BO1E, 87DOZY, 87GI1B, 87GI1C, 87GO05, 87KA39, 87KO1O, 87LE1E, 87NA04, 87RO23, 88GIZU, 88KO1V, 88MI1K, 88OH04, 88TI06, 89BA63, 89CH31, 89DI1B, 89DO1L, 89GA09, 89GE10, 89GIZW, 89GIZV, 89IT04, 89KH1E, 89NA01, 89RI05, 90BE24, 90CH12, 90CH1S, 90DI1D, 90ER03, 90ER1E, 90GH01) Kaon capture and reactions: (85BE62, 86BE42, 86DA1G, 86FE1A, 86MA1C, 86WU1C, 89BEXX, 89BEXU, 89DO1I, 89DO1K, 89SI09) Antinucleon reactions: 87PO05, 89RI05, 90JO01) (86BA2W, 86KO1E, 86RO23, 86SP01, 87AH1A, 87GR20, 87HA1J, 27
- Page 1 and 2: 14 Revised Manuscript 06 November 2
- Page 3 and 4: 14 He (Not illustrated) 14 He has n
- Page 5 and 6: Figure 1: Energy levels of 14 B. Fo
- Page 7 and 8: 5. 14 C( 14 C, 14 N) 14 B Q m = −
- Page 9 and 10: Table 14.3: Energy Levels of 14 C a
- Page 11: a See also Tables 14.8 here and in
- Page 14 and 15: a (73AJ01): E( 6 Li) = 20 MeV. See
- Page 16 and 17: Table 14.5: States in 14 Cfrom 11 B
- Page 18 and 19: for 14 C*(8.32) is 215 +84 −35 me
- Page 20 and 21: correspond to single states, and th
- Page 22 and 23: 19. 13 C( 13 C, 12 C) 14 C Q m =3.2
- Page 24 and 25: Table 14.9: States of 14 Cfrom 14 C
- Page 28 and 29: Table 14.10: Energy Levels of 14 N
- Page 30 and 31: Table 14.10: Energy Levels of 14 N
- Page 32 and 33: Table 14.10: Energy Levels of 14 N
- Page 34 and 35: a See also Tables 14.15 and 14.13,
- Page 36 and 37: Table 14.11: Radiative decays in 14
- Page 38 and 39: Table 14.11: Radiative decays in 14
- Page 40 and 41: Table 14.12: Resonances in 10 B+α
- Page 42 and 43: functions for the transitions to 8
- Page 44 and 45: Table 14.13: Resonances in 12 C+d a
- Page 46 and 47: Table 14.14: States of 14 Nfrom 12
- Page 48 and 49: Table 14.15: States in 14 Nfrom 10
- Page 50 and 51: Table 14.16: Levels of 14 Nfrom 13
- Page 52 and 53: Observed resonances are displayed i
- Page 54 and 55: For searches for short-lived neutra
- Page 56 and 57: a See also Table 14.18 in (81AJ01)
- Page 58 and 59: Angular distributions have been stu
- Page 60 and 61: Form factors have been determined a
- Page 62 and 63: 46. 14 N(d, d) 14 N Angular distrib
- Page 64 and 65: 56. (a) 14 N( 24 Mg, 24 Mg) 14 N (b
- Page 66 and 67: Table 14.21: States of 14 Nfrom 15
- Page 68 and 69: 14 O (Figs. 4 and 5) GENERAL (See a
- Page 70 and 71: Table 14.22: Energy levels of 14 O
- Page 72 and 73: structure near 23 MeV is also obser
- Page 74 and 75: Figure 5: Isobar diagram, A=14. The
- Page 76 and 77:
78MO08 S. Mordechai, H.T. Fortune,
- Page 78 and 79:
84PE1B Peterson et al, Nucl. Phys.
- Page 80 and 81:
85HO21 E. Hourani, M. Hussonnois, L
- Page 82 and 83:
85WA22 S. Wald, S.B. Gazes, C.R. Al
- Page 84 and 85:
86CU02 B. Cujec, B. Dasmahapatra, Q
- Page 86 and 87:
86KO08 P. Kozma and P. Bem, Czech.
- Page 88 and 89:
86SH25 B. Shivakumar, D. Shapira, P
- Page 90 and 91:
87AJ02 F. Ajzenberg-Selove, Nucl. P
- Page 92 and 93:
87DOZY B. Doyle, R. Wittmann and N.
- Page 94 and 95:
87KU1C Kubozoe and Watanabe, Nucl.
- Page 96 and 97:
87ROZY S.H. Rokni, H.W. Baer, J.D.
- Page 98 and 99:
88AN19 A. Antonov, V.A. Vesna, Yu.M
- Page 100 and 101:
88GO12 M. Gonin, J.P. Coffin, G. Gu
- Page 102 and 103:
88OS1A Oset et al, AIP Conf. Proc.
- Page 104 and 105:
88WO04 A.A. Wolters, A.G.M. van Hee
- Page 106 and 107:
89CA15 S. Cavallaro, S.Z. Yin, G. P
- Page 108 and 109:
89GU28 N. Guessoum and R.J. Gould,
- Page 110 and 111:
89PO07 J. Pouliot, Y. Chan, A. Daca
- Page 112 and 113:
89VA21 D. Vartsky, M.B. Goldberg, G
- Page 114 and 115:
90HA46 D. Harley, B. Müller and J.
- Page 116:
90WIZV 90YA01 90YA02 90YE02 HA80F V