|
![]() |
![]() |
![]()
18O (1995TI07)(See Energy Level Diagrams for 18O)
GENERAL: See .
< r2 >1/2 = 2.784 ± 0.020 fm: see reaction 25. g = -0.287 ± 0.015 [see (1983AJ01)]. Q = -0.042 ± 0.008 b [weighted mean of -0.036 ± 0.009 and -0.058 ± 0.015 b: see (1983GR28); see also (1983AJ01)].
For a discussion of the hexadecapole deformation see (1983GR10). See also (1987RA01).
Reactions (a) and (b) have been studied by (1993CU01, 1993DA17) in low energy heavy-ion fusion reactions. It is reported that the ≈ 3 MeV wide resonance observed at Ex(18O) ≈ 28 MeV in the 7Li + 11B → 18O → 16O + nn and 9Be + 9Be → 18O → 16O + nn reactions overlap with the higher part of the T< = 1, 18O GDR observed in photonuclear excitation.
See (1986CU02) for production cross sections of 1.98 MeV γ-rays.
Observed proton groups are displayed in In a recent experiment, the 4+ state at 7117 keV in 18O was studied by (1994ME02) and an E2 strength for the 7117 - 5060 branches of B(E2) = 6.4 ± 1.6 W.u. was deduced in agreement with results of (1989GA01). It was concluded that it is highly improbable that the 7117 keV state is energetically degenerate with a state of different decay properties.
See (1986SM01) and
Resonances in the yield of capture γ-rays are observed at
Eα = 1.14, 1.79, 2.09, 2.33, 2.44, 2.55, and 2.64 MeV: see
The 14C(α, γ) reaction is important in astrophysical processes and the details of the cross section are relevant to the process of heavy element formation in inhomogeneous big bang nucleosynthesis (1988AP1A, 1989FU06, 1990WIZP, 1992GA11, 1992GO14). See also (1988BU01, 1988MA1U, 1989KA1K, 1989NO1A, 1989TH1C) and the review of thermonuclear reaction rates in (1988CA26).
Observed anomalies in the scattering [reaction (a)] for Eα =
2 to 8.2 MeV and the resonances in the relative neutron yield [reaction (b)]
for Eα = 2.3 MeV are displayed in The α-cluster structure of 18O has been investigated in theoretical work of (1989FU08, 1993RE03) based on 14C(α, α) scattering, and the results do not support the existence of proposed negative-parity molecular dipole states. See (1989GA01).
At E(6Li) = 34 MeV angular distributions have been measured for the deuteron groups to many states of 18O (1981CU07) [see also (1983AJ01)] including 18O*(17.6 ± 0.2) (1982CU01). Jπ = 4+, 2+, 2+, (4+), and (4+) are suggested for 18O*(7.86, 8.9, 12.04, 14.6, 17.0) (1981CU07). The 2+, 4+, 6+ and 8+ members of the Kπ = 0+2 rotational band based on 18O*(3.62) are 18O*(5.26, 7.12, 11.69, 17.6) (1982CU01). Angular correlations have been measured at E(6Li) = 34 MeV; these lead to the assignment of Jπ = 8+ to 18O*(17.6) (1982CU01) and to the assignment of Jπ = 4+, 5-, 6+, 7- and 8+ to sixteen states in 18O with 11.4 ≤ Ex ≤ 23.1 MeV (1983CU03) [see (1983CU03) for assignment of 18O states to bands]. At E(6Li) = 32 MeV (1983AR11) find that the strongest groups are those to (unresolved) structures at Ex = 17.05 and 18.95 MeV [each Γ ≈ 0.35 MeV] dominated by Jπ = 7-. 18O*(11.6, 12.6) with Jπ = (6+, 5-) and 5- are also observed (1983AR11) [see, however, the density of states]. See also (1987AJ02, 1990OS03).
At E(7Li) = 20.4 MeV, triton groups are observed corresponding to a number of states of 18O with Ex < 12.6 MeV. Angular distributions were obtained for some of these, including 18O*(0, 1.98, 7.12, 11.69) with Jπ = 0+, 2+, 4+, 6+. The latter two are the most strongly populated in this reaction: they appear to be part of the ground-state rotational band: see (1972AJ02). See also (1987AJ02).
In more recent work at E(7Li) = 15 MeV, 18O
gamma de-excitation modes for all natural parity states up to the
alpha-particle threshold at Ex = 6.227 MeV were studied (1991GA08).
See
See (1985KO04).
See (1978AJ03).
Several states in 18O at Ex = 10 - 25 MeV were observed in 15N(α, p) experiments reported in (1987MIZY, 1988BRZY, 1989BR1J).
See (1983AJ01).
Proton groups corresponding to states of 18O are displayed in
At Eα = 65 MeV, the angular distribution to 18O*(3.55) [Jπ = 4+] has been studied. 18O*(8.04, 9.15, 10.3) are also populated: see (1983AJ01).
At E(10B) = 100 MeV, 18O*(3.55) [first (d5/2)24+ state] is preferentially populated. 18O*(1.98, 5.26, 7.12, 8.0, 8.3, 9.1) are also observed. The angular distribution to 18O*(3.55) has been measured at E(13C) = 105 MeV. See (1983AJ01, 1983OS07).
For reaction (a) see (1983AJ01). [The work reported there has not been published.] The scattering amplitude (bound) a = 5.62 ± 0.45 fm, σfree = 3.55 ± 0.25 b. The thermal cross section for reaction (c) is 235 ± 10 mb. See (1983AJ01) for references. See also (1988MCZT). In more recent work, the cross section for 17O(n, α) has been measured from En = 25 × 10-3 eV to 1 MeV (1991KO31). An evaluation of the cross sections from En = 10-5 eV to 20 MeV has been carried out by (1991HI15). Results are given in tabular and graphical form. See also (1991KO1P).
Observed proton groups are displayed in
Differential cross sections were measured at Eα = 65 MeV (1992YA08) for
18O states up to Ex = 15 MeV. DWBA analysis led to
proposed spin parity and isospin assignments, and spectroscopic factors. See
Angular distributions involving 18O*(0, 1.98, 3.55) have been studied at E(12C) = 115 MeV: see (1983AJ01).
The transitions observed in the β- decay are displayed in
The γ-decaying states were measured by (1982OL01) and
estimated 15 ± 6% branching to non-γ-decaying states in
18O was assumed. At least 12.2 ± 0.6% of the β-decay
branching ratio has been measured to feed 1- alpha-particle
emitting states (1989ZH04). See
also the measurements of (1987GAZW, 1987ZHZV, 1988MI1G). A β-delayed
neutron emission probability of 14.3 ± 2.0% has been measured (1991RE02). The
β- branchings to γ-emitting states of (1982OL01) has
been renormalized to take in account the 26.5 ± 2.1% branches to
particle emitting states. The γ-ray intensities of (1982OL01) also
need to be renormalized by this factor, see
The cross sections for the (γ, p), (γ, n), (γ, 2n) and
(γ, tot) [tot = total absorption] have been measured with monoenergetic
photons to 42 MeV: observed resonances are displayed in In a related, but more recent, experiment the cross section for reaction (e) was measured (1991MC01) and it was determined that the cross section rises to a maximum of 1.2 mb at 27.5 MeV, approximately one-tenth of the total (γ, n) cross section there. The cross section integrated to 43 MeV is only 11.8 mb · MeV, and as a result the isospin assignments of (1979WO04) are unaffected by neglect of this channel. A recent extensive study of isospin effects in the photodisintegration of light nuclei (1993MC02) used a collection of data on (γ, p), (γ, n), (γ, 2n) and (γ, n0) cross sections and separated the T> and T< isospin components of the GDR in several light nuclei including 18O. The relative strengths were extracted. See also the atlas of photoneutron cross sections with monoenergetic photons (1988DI02), and see (1988BE1T, 1989NO1C). Structures in the (γ, α0) cross section are reported at Ex = 18.2, 20.9, 22.1, and 24.2 MeV (1982BA03; Ebrems.). The decay of the GDR to 14C, 15N, 16O, 17N and 17O states has been studied: see (1983AJ01). Less than 20% of the decay of states with 14.5 < Ex < 20 MeV goes via the n0 channel (1987JU07). See (1978AJ03, 1987AJ02) for the earlier work.
For 18O*(6.20) Γγ0 = 0.18 ± 0.03 eV, assuming Γγ0/Γ = 0.88; Ex = 6202.7 ± 0.8 keV: see (1978AJ03).
The 18O charge radius, < r2 >1/2 = 2.784 ± 0.020 fm, based on studies of the elastic charge form factors for Ee = 70 to 370 MeV, the resulting determinations of the difference in the 18O and 16O radii, and the rms radius of 16O: see (1983AJ01).
Inelastic scattering has been reported to many states of 18O: see
(1983AJ01, 1987AJ02) and Several theoretical studies of inelastic electron scattering to states of 18O have been carried out. A microscopic calculation for scattering to 2+ states is reported in (1988HAZZ) and to 0+ and 2+ states in (1988KU17). See also the calculations of transition charge densities described in (1988GU03, 1988GU12, 1992GU11) and see (1987GU1D, 1988GU1B, 1989AJ1A).
Angular distributions for the scattering to 18O*(0, 1.98, 5.10) have been reported at Eπ± = 29.2 to 230 MeV [see (1983AJ01)] and at 50 MeV (1984TA1A; 18O*(0, 1.98)) at 140, 180, and 220 MeV (1984SE1A; 18O*(1.98)), at 164 MeV (1987CH14; 18O*(0, 1.98, 4.46, 5.10)) and (1988SE04; 18O*(1.98, 3.92, 5.26 MeV)). See also (1989GR1M, 1990WI1K). Measurements and analysis work reported in (1983AJ01) determine < rn2 >1/2 = 2.81 ± 0.03 fm, < rn2 >1/2 - < rp2 >1/2 = 0.03 ± 0.03 fm. For a discussion of proton matter distribution in 18O see (1985BA27). Total reaction cross sections at Eπ = 50 MeV have been determined by (1987ME12). At E = 165 MeV, the cross section for reaction (c) is larger for 18O than for 16O while reaction (b) has a lower cross section (1982PI06). For the (π+, 2p), (π+, pn) and (π-, pn) reactions at Eπ = 165 MeV see (1984AL20, 1986AL22). Results of Glauber model calculations of pion scattering from 18O at energies above the Δ33 resonance are presented in (1991OS01). A microscopic study of inelastic scattering to the 2+ states in 18O is reported in (1988HAZZ). See also the review of pion-nucleus physics in (1991MO13).
Angular distributions have been measured for En = 2.9 to 24 MeV [see (1972AJ02, 1983AJ01)] and at En = 5.0 to 7.5 MeV (1986KO10; n0, n1).
Angular distributions have been measured for Ep = 0.84 to 135 MeV [see (1978AJ03, 1983AJ01)], at Ep = 135 MeV (1986KE05; p1) and at Ep = 800 MeV (1982GL08; p to 18O*(0, 1.98, 7.12).) At Ep = 24.5 MeV (1974ES02) have studied the angular distributions of the proton groups to 18O*(1.98, 3.55, 3.63, 3.92, 4.46, 5.10, 5.26, 5.53, 7.12): a modified DWBA analysis leads to Jπ = 2+, 4+, 0+, 2+, 1-, 3-, 2+, 2- and 4+ for these states. A coupled-channels calculation suggests β2 = 0.37 ± 0.03, 0.56 ± 0.06 and 0.18 ± 0.04 for 18O*(1.98, 5.10, 7.12). Such calculations also support evidence for a rotational band involving 18O*(0, 1.98, 7.12). The 3- state at 5.10 MeV is strongly excited and collective in nature: B(E3) = 1120 e2 · fm6. For 18O*(1.98, 3.92, 5.26), B(E2) = 45, 8.3 and 24 e2 · fm4 (1974ES02). The 800 MeV data indicates that 18O*(7.12) can be described only if a large hexadecapole deformation is assumed (1982GL08). At Ep = 201 MeV, σ(θ) at forward angles has been measured to 18O*(8.21, 8.82, 16.40): it is proposed that 18O*(8.82) has Jπ = 1+ and that additional 1+ strength is located in a group centered at Ex ≈ 10.1 MeV as well as in the region Ex = 12.4 to 15 MeV. The 1+; T = 2 state 18O*(18.87), reported in (e, e'), is not observed (1987DJ01). See also (1988CR1B). 18O*(1.98) has |g| = 0.287 ± 0.015 [τm = 2.99 ± 0.12 ps]. 18O*(3.55) has |g| = 0.62 ± 0.10 suggesting a mainly (d5/2)2 configuration for this state: see (1983AJ01). See also 19F and (1987AJ02). A Dirac optical model analysis of 18O(p, p) cross section and analyzing power at 800 MeV is described in (1990PH02). A coupled-channels analysis was presented in (1988DE31). The intrinsic radial sensitivity of nucleon inelastic scattering was studied by (1988KE01) and a comparison of electromagnetic and hadronic probes of nuclear structures is described in (1986KE1C).
Angular distributions are reported with 178.4 MeV antiprotons to 18O*(0, 1.98) (1986BR04, 1986LE13). For atomic effects see (1986KO22). See also (1987AJ02). Differential cross sections for elastic and inelastic scattering of 180 MeV antiprotons by 18O were calculated in the eikonal and Glauber approaches by (1992TA08).
Angular distributions have been reported at Ed = 7.0 to 15.0 MeV: see (1972AJ02, 1983AJ01). See also 20F.
See (1972AJ02).
The elastic scattering has been studied at E(3He) = 11.0 to 41 MeV [see (1972AJ02, 1983AJ01)] and at 14 MeV (1982AB04), at 25 MeV (1982VE13) [the matter radius, < r2 >1/2m = 2.59 ± 0.12 fm] and at 33 MeV (1983LE03; also Aγ; and also to 18O*(1.98)). A strong-absorption model analysis of angular distributions at 2.5 and 41 MeV is described in (1987RA36). See also (1985HA11, 1987CO07).
Recent elastic scattering cross sections at Eα = 44.8 MeV
were reported by (1992AR18).
Angular distributions of many α-groups have been measured in the range
Eα = 21 to 40.5 MeV [see (1978AJ03)], at 23.5 MeV (1984SA28; to
18O*(1.98, 3.56 + 3.63, 3.92, 4.45, 5.1 - 5.53)) and at 54.1 MeV
(1987AB03;
g.s.). The transitions to 18O*(4.46, 5.10) are L = 1 and 3,
respectively, fixing Jπ = 1- and 3- for
these states. Measurements of α-groups near 180° for
Eα = 20.0 to 23.4 MeV confirm assignments of natural parity
for 18O*(1.98, 3.55, 3.63, 3.92, 4.46, 5.10, 5.26, 5.34, 6.20,
6.40, 7.12, 7.62, 7.86, 8.22, 8.29, 8.82, 8.96, 9.03, 9.10, 9.36, 9.41, 9.67,
9.72 ± 0.03, 9.88, 10.12, 10.30, 10.40, 11.62, 11.69). [See, however,
Alpha-gamma correlation measurements involving 18O states below
Ex = 6.4 MeV [see
A recent search for a bound system of π- and neutrons in the fragmentation region of 18O + 9Be collisions at 100 A · MeV is reported in (1993SU08). Upper limits were obtained. See also (1972AJ02, 1987AJ02).
An elastic angular distribution has been reported at E(11B) = 115 MeV: see (1983AJ01). For reaction (a) see (1974AJ01). A recent measurement of 18O on 10, 11B targets at Elab ≈ 55 MeV is described in (1993AN08) and evidence for fusion-fission rather than orbiting is reported. See also (1990SZ1C).
Elastic angular distributions have been studied at E(18O) = 32.3 to 57.5 MeV for reaction (a) [as well as at E(18O) = 70, 100, and 140 MeV (1982HE07)] and at E(18O) = 31 MeV for reaction (b). Yields and fusion cross sections are reported by (1982BA49, 1982HE07, 1985BE40, 1985CA01, 1986GA13). For reaction (c) see (1986STZY). See also (1983AJ01, 1987AJ02). Angular correlations (reaction (d)) have been studied at E(18O) = 82 MeV. 18O*(7.10, 7.62, 7.86, 8.04, 8.22, 10.30, 11.59, 12.55) are observed: the first seven of these have Jπ = 4+, 1-, 5-, 1-, 2+, 4+, 5- (1984BH01, 1984RA07). In addition 18O*(9.33, 9.65) are also populated [Γ ≈ 0.3 MeV]: a possible interpretation of the data is that these two are 3- states and that there is in addition a very wide (> 1 MeV) 2+ state at ≈ 9.5 MeV (1984RA17). See also (1987AJ02). Giant dipole decays in nuclei excited by 18O + 12C collisions were discussed in (1989BEZC, 1990SN1A). Competition between p2n, dn and t emissions in the 12C + 18O reaction was studied in an experiment reported in (1990XE01). Predictions of possible resonant behavior in medium-mass colliding systems are discussed in (1989CI1C). Molecular single particle effects for 12C + 18O are explored in calculations described in (1987MO27).
See (1983DU13).
Angular distributions have been measured at many energies for E(16O) = 24 to 54.5 MeV and E(18O) = 25 to 52 MeV, involving besides 18Og.s., 18O*(1.98, 3.55 + 3.63, 3.92, 4.46, 5.10, 7.12). At E(18O) = 126 MeV 18O*(9.0) is relatively strongly populated. See (1983AJ01). For yields and fusion cross sections, including the effect of 18O*(1.98), see (1985TH03, 1985WU03, 1986GA13, 1986TH01). See also (1987AJ02). Competition between p2n, dn and t emissions in 18O + 16O reactions was studied in an experiment reported in (1990XE01). A unified description of sub-barrier interactions of oxygen isotopes is discussed in (1987PO11); see the coupled-channels calculations reported in (1992LI1K). See also the review of sub-barrier fusion in (1988BE1W). A semi-classical analysis of two particle transfer in 16O + 18O reactions is discussed in (1987MA22).
Angular distributions involving 18O*(0, 1.98) are reported at E(17O) = 36 MeV. Angular distributions [reaction (b)] have been studied at E(18O) = 20 to 52 MeV. 18O*(3.55 + 3.63, 4.46, 5.10, 7.12) are also populated; see (1978AJ03, 1983AJ01). See also (1987AJ02) and see (1990XE01) reporting on p2n, dn and t emissions in 18O + 18O reactions. The effect of high spin states on fusion in 18O + 18O systems has been studied in the framework of a statistical theory (1987RA28).
The elastic scattering has been studied at E(19F) = 27, 30, and 33 MeV: see (1983AJ01). See also (1987AJ02). An experiment reported in (1990XE01) studied p2n, dn and t emission in 18O + 19F reactions.
Angular distributions are reported for reaction (a) at E(18O) = 29 and 35 MeV to 18O*(0, 1.98). See (1987AJ02).
The elastic angular distribution has been studied at E(18O) = 100 MeV (1981ME13). See also (1983AJ01, 1987AJ02).
Elastic angular distributions are reported at E(18O) = 36 to 56 MeV [see (1983AJ01)] and at 351.7 MeV (1984BUZX, 1988BU15; also to 18O*(1.98)). See also (1987AJ02). Ambiguities in optical-model potentials for describing 18O + 28Si and other heavy-ion reactions are discussed in (1987HO18). See also (1989NA1M).
Angular distributions have been measured at E(18O) = 62.1 MeV [reaction (a)] for the transitions to 18O*(0, 1.98, 5.10) (1982RE14). For a fusion study [reaction (b)] see (1984DE38). See also (1987AJ02, 1987SC34).
See 18F.
(1985KE03) have measured the yields of proton groups to 18O*(0, 1.98) [and to unresolved states] for Ebs in the GDR range. See also (1978AJ03) and 19F.
Angular distributions have been measured at En = 14 to 14.4 MeV: see (1972AJ02). See also (1978AJ03) and 20F. Nuclear model calculations for En = 2 - 20 MeV are described in (1992ZH15).
Experimental and theoretical studies of knockout reactions are reviewed in (1987VD1A).
Many states of 18O (Ex < 14.6 MeV) have been populated
in this reaction: see
At Ed = 80 MeV angular distributions have been measured for the 6Li groups to the ground state of 18O and to excited states at 1.98, 3.57, 5.10, 6.30, 7.8, 9.4 [ ± 0.04] MeV (1984OE02) [see also for Srel.]. For the earlier work see (1983AJ01).
|
![]() |