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15O (1991AJ01)(See Energy Level Diagrams for 15O)
GENERAL: See also (1986AJ01), Nuclear models:(1987ST05). Special states:(1985SH24, 1986LI1B, 1987ST05, 1988AN1E, 1989WU1C). Electromagnetic transitions:(1984VA06, 1987HO1L, 1987ST05). Astrophysical questions:(1985TA1A, 1987RA1D, 1989JI1A, 1989ST14, 1990RA1O). Complex reactions involving 15O:(1985FI08, 1985HU1C, 1985PO11, 1985SI19, 1986GR1A, 1986ME06, 1986PO06, 1986TO10, 1986UT01, 1987BA38, 1987BE1I, 1987BU07, 1987NA01, 1987RI03, 1987ST01, 1988BE02, 1988BE56, 1988MI28, 1989BA92, 1989CA25, 1989DR03, 1989KI13, 1989PO07, 1989SA10, 1989TA1O, 1989YO02). Applied work:(1985BO1P, 1985HA40, 1987HI1B, 1988HI1F, 1988VO1D, 1989AR1J, 1989WO1B). Pion and other mesons capture and reactions (See also reactions 8, 16, 17 and 21.): (1986LI1B, 1987LE1B, 1988CH49, 1988MI1K, 1989LE1L, 1990OD1A). Hypernuclei:(1984ZH1B, 1986DA1G, 1989BA93, 1989KO1H, 1989TA17). Other topics:(1985AN28, 1985SH24, 1986AN07, 1986WI03, 1987CH02, 1989WU1C, 1990MU10). Ground-state properties of 15O:(1985AN28, 1985AR11, 1986MC13, 1986WI03, 1986WUZX, 1987FU06, 1987SA15, 1988AR1B, 1988CH1T, 1988FU04, 1988NI05, 1988SH07, 1988VA03, 1988WA08, 1989CH24, 1989FU05, 1989NE02, 1989SA10).
15O*(5.24): μ = +(0.65 ± 0.07) nm: see (1989RA17).
The half-life of 15O is 122.24 ± 0.16 s: see (1981AJ01); log f0t = 3.637. The K/β+ ratio is (10.7 ± 0.6) × 10-4: see (1976AJ04). The β-anisotropy has been measured by (1988SE11, 1989DE07). See also (1986AJ01), (1990ST08), (1985BA1N, 1985BA1M, 1986GR04, 1987BA89, 1987FR1C, 1987RI1E, 1987WE1C, 1988BA86, 1988BA1Y, 1989BA2P, 1989DA1H; astrophysics) and (1988TA09, 1988TO1C, 1989WO1E; theor.).
For reaction (a) see (1986BE54); for reaction (b) see (1986BE35). For other heavy-ion reactions see (1986AJ01).
Excitation functions and polarization measurements for these reactions have been
measured over a wide range of energies: see
The 90° yield and the angular distributions of γ0, measured from E(3He) = 5.24
to 13.95 MeV show five resonances attributed to E1 transitions from Jπ = 1/2+ or 3/2+, T = 1/2 states
in the GDR characterized by a considerable 3p4h admixture ((1978DE33) [also for
ωγ], (1984DE09)). Yields of
γ1+2 at 90° have also been reported at
E(3He) = 5.3 to 16.7 MeV: the cross section is some eight times
greater than that for (3He, γ0)
and is similar to that for the The yield of n0 (reaction (b)) shows resonances for E(3He) < 10 MeV and little structure above, to 30.6 MeV: see (1981AJ01) [n1 and n2+3+4 yields are also reported]. The yield of protons (reaction (c)) shows some clear resonances below E(3He) = 4.5 MeV and some uncorrelated structures at higher energies (to E(3He) = 12 MeV) with the possible exception of states at Eres = 7.8, 9.2 - 9.6 and (10.5) MeV. For E(3He) = 16 to 30.6 MeV no appreciable structure is observed in the p0, p1 and p2 yields: see (1976AJ04). At E(3pol. He) = 33 MeV Ay has been measured for 14N*(0, 2.31, 3.95): see (1986AJ01). For polarization effects in the (3He, 2p) reaction at E(3pol. He) = 33 MeV see (1986KA44). For reactions (d) and (e) see (1976AJ04, 1981AJ01, 1986AJ01). The elastic scattering (reaction (f)) shows some resonant structure near 3, 5 and 6 MeV and some largely uncorrelated structures in the range E(3He) = 16.5 to 24 MeV. There is some suggestion, however, of two resonances at E(3He) = 17 and 20 MeV: see (1976AJ04). Resonance-like behavior is also reported at E(3pol. He) = 29 MeV. Polarization measurements are reported for E(3pol. He) = 20.5 to 32.6 MeV: see (1981AJ01). See also (1986AJ01). The yield of α-particles displays resonance structure below 8 MeV, and broad fluctuations for E(3He) = 12 to 18.6 MeV: see (1976AJ04). Polarization measurements are reported for E(3pol. He) = 33.3 MeV for the α0 and α1 groups: see (1981AJ01). For Ay measurements of the (3He, 7Be) and (3He, 6Li) reactions see (1989SI02, 1986CL1B). For π± production see (1986MI25). For a search for subthreshold K+ production see (1985IA01). For work at very high energies see (1985AB1B, 1985AD1C). See also (1986AJ01), (1984NA1F), (1990TO10; applied) and (1986EV01, 1986SI02; theor.).
Angular distributions of the n0 group have been measured for Eα = 18.4 to 23.1 MeV: see (1976AJ04). At Eα = 41 MeV angular distributions are reported to 15O*(5.24, 6.86 + 7.28, 9.63[u], 10.48[u], 11.72[u], 12.85[u], 15.05[u]). 15O*(8.92, 11.1, 12.3, 13.45, 13.72, 14.27, 15.65) are also populated ((1981OV01) [uncertainties in Ex are not shown; unresolved states are a problem]). At Eα = 47.4 MeV groups are populated at θ = 0° corresponding to 15Og.s. and to unresolved states at 5.2, 7.3, 10.0, 12.5 and 15.3 MeV (1988LU02). See also (1988CA26; astrophys.).
States observed in this reaction are displayed in
At E(12C) = 187 MeV, θlab = 8°, the spectrum is dominated by 15O*(12.84, 15.05) [assumed Jπ = 1/2-, 13/2+, respectively]. 15O*(7.28) [Jπ = 7/2+] is populated but 15O*(0, 6.79) are not observed. The situation is similar at E(12C) = 114 MeV but at E(12C) = 72 MeV (θlab = 11°) 15O*(0, 5.2, 7.28) are populated with comparable intensities: see (1976AJ04). At E(12C) = 480 MeV the three most strongly excited states in the forward direction are 15O*(10.46, 12.83[u], 15.05[u]) [Jπ = 9/2+, 11/2-, 13/2+] and forward angle σ(θ) have been measured. 15O*(0, 5.24, 7.3, 8.9[u], 16.7[u], 18.2[u], 21.1[u], 22.1[u]) are also populated (1988KR11).
Observed groups are displayed in
At Epol. p = 183 MeV differential cross sections and Ay are reported for the transitions to 15O*(0, 7.3), the two states strongly populated in the reaction (1982JA05, 1982VI05). See also (1986JA1H) and (1986KU1J, 1990KU1H; theor.).
Observed resonances in the yield of γ-rays are listed in
(1987SC1H) have studied absolute cross sections, γ-ray angular distributions and excitation functions for Ep = 0.2 to 3.6 MeV: S(0) is determined to be 3.20 ± 0.54 keV · b. C2S are derived for the first eight states of 15O (1987SC1H). The 90° γ0 yield has been measured for Ep = 2.2 to 19 MeV: resonances are observed over most of the range. The (γ1 + γ2) yield is relatively weak. For Ep = 18 to 28 MeV the excitation function for γ0 decreases smoothly with energy: there is no evidence for structures [see (1981AJ01)]. See also (1985CA41, 1987KR04, 1987WE1C, 1988CA1J, 1988CA26, 1989BA2P, 1989TH1C, 1990MA1P; astrophysics) and (1990HA46; theor.).
The excitation function has been measured for Ep = 6.3 to 12 MeV: see
(1970AJ04). Observed resonances
are displayed in
The yields of elastic and inelastic protons, and of 2.31 MeV γ-rays, have been studied at many energies: see (1959AJ76, 1970AJ04, 1976AJ04). Observed resonances are
displayed in Polarization measurements have been carried out at Ep = 3.0 to 159.4 MeV [see (1970AJ04, 1976AJ04, 1986AJ01)] and at Epol. p = 35 MeV (1990IE01; p1) and 0.8 GeV (1985BL22; Ay; elastic). See also 14N, (1986BA2U), (1986BA88, 1987HU01) and (1989AM01; theor.).
Excitation functions for the ground-state group have been measured at Ep
= 7 to 11 MeV: some resonant structure is indicated [see
Excitation functions and total cross-section measurements have been measured for
the α0 group for Ep = 3.8 to 45
MeV: see (1976AJ04). Fairly sharp
structures persist until Ep = 15 MeV: see
Angular distributions have been studied at many energies in the range Ed
= 0.9 to 11.8 MeV: see
See
At Eγ = 170 MeV four-point angular distributions of the π- to 15Og.s. have been measured by (1988LI23) and (1989KO28): the two studies are not in good agreement. See also (1990ER03; theor.).
Angular distributions of the π0 to 15Og.s. have been studied at Eπ+ = 32.4 and 55.5 MeV (1985IR02), at 48 MeV (1984CO04, 1986LE01) and at 165 MeV (1982DO10). Forward-angle differential cross sections of the π0 to 15Og.s. have also been measured at Eπ+ = 20 MeV (1987IR01) and at 40.7 and 63.6 MeV (1985IR02). See also (1989LE1L).
Angular distributions have been measured for Ep = 3.95 to 18.5 MeV [see (1981AJ01, 1986AJ01)], at 35 MeV (1987OR01; 15O*(7.56) [Jπ = 1/2+]), at 135 MeV (1985WA24; 15O*(0, 6.2)) and at 200 and 494 MeV (1988CIZZ; prelim.; also Ay). Forward-angle differential cross sections at Ep = 200, 300 and 400 MeV to 15O*(0, 6.2) are reported by (1987ALZW; prelim.). The ratio of the population of 15Og.s. to that of 15O*(6.2) has been determined at Ep = 800 MeV (1986KI12). 15O*(6.2) contains only about 1/3 of the expected GT strength (1985GO02). [I am indebted to Prof. C.D. Goodman for his comments.] For a discussion of GT strengths, see (1987TA13). 15O*(5.2[u], 6.8[u], 7.28) have also been populated (1987OR01). For the earlier work see (1986AJ01). See also 16O in (1986AJ04), (1985GO1Q, 1986VO1G, 1987BE25, 1988RO17, 1988WA1Q), (1986MA1P, 1987HI1B, 1988HI1F; applied) and (1989RA15; theor.).
Angular distributions for the t0, t1+2, t3, t4+5, t6 and t7 groups have been studied for E(3He) = 16.5 to 44.6 MeV: see (1976AJ04).
The spectrum of photoneutrons has been investigated at many energies. Measurements over the giant dipole resonance region show the predominant strength is to the Jπ = 1/2- and 3/2- states Ex = 0 and 6.18 MeV, consistent with the basic validity of the single-particle, single-hole theory of photoexcitation in 16O. However, the positive-parity states at Ex = 5.18, 5.24, 6.86 MeV are also populated suggesting some more complicated excitations in 16O: (1970AJ04, 1976AJ04). Differential cross sections for the n0 group have been measured from threshold to Eγ = 28 MeV [see (1976AJ04)], at Eγ = 60 to 160 MeV (also 15O*(6.18); no appreciable strength in the 5.2 MeV doublet) [see (1986AJ01)] and at 150, 200 and 250 MeV (1989BE14). See also 16O in (1986AJ04) and (1987RY03, 1988CA10, 1988DUZX, 1988RY03, 1990BRZY, 1990FL1A; theor.).
For reaction (a) see (1982DO01). At Eπ+ = 2.0 GeV/c differential cross sections have been determined for the transition to 15N*(6.2) (1983KI01) in reaction (b). For reaction (c), see (1986GI1A).
At Ep = 505 MeV the summed spectra show two peaks corresponding to the p1/2 and p3/2 knockouts [15O*(0, 6.18)] (binding energies of 15.64 and 21.82 MeV). Differential cross sections are also reported (1986MC10) [see also reaction 59 in 15N]. For work at 1 GeV, see (1985BE30). See also (1983WA1C) and (1987HI1B; applied).
Angular distributions have been reported at many energies for Ep = 18.5
to 155.6 MeV [see For γ-ray production [15O*(5.24)] see (1988LE08). See also 17F in (1986AJ04), (1989WA16) and (1987LA11, 1988LE08, 1989GU28; astrophysics).
Angular distributions have been reported at a number of energies in the range Ed = 20 to 52 MeV [see (1981AJ01) and reaction 60 in 15N here] and at Epol. d = 89 MeV (1990SA27; 15O*(0, 6.18)). See also 18F in (1983AJ01).
The p1/2 and p3/2 hole states 15O*(0, 6.18) are
strongly populated. Information on these and other states are displayed in
See (1986GL1E; prelim.).
At Ep = 39.8 MeV angular distributions of t0 and t3 groups have been compared to those of the 3He groups to the analog states in 15N. At Ep = 45 MeV a state, assumed to be the Jπ = 5/2+, T = 3/2 analog of 15C*(0.74), is observed at Ex = 12.255 ± 0.013 MeV, Γc.m. = 135 ± 15 keV. The state decays by proton emission to the T = 1, 0+ state 14N*(2.31) [the population of some T = 1/2 states is also reported]: see (1981AJ01). Epol. p = 89.7 MeV angular distributions and Ay measurements have been reported to 15O*(0, 5.24[u], 6.18, 6.86, 7.28) (1985VO12).
See (1976AJ04). See also (1986HA1E; theor.).
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