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1.
《Nuclear Physics A》1987,465(3):445-460
The 48Ca(t, α)47 K reaction has been measured at 33 MeV bombarding energy. Spectroscopic information has been extracted for 13 states in 47K and 9 new levels have been observed in this nucleus. A comparison of Spectroscopic factors is made with a recent shell-model calculation and the presence of proton core-excitations in the ground state of 48Ca is examined.  相似文献   

2.
In a high resolution48Ca(d,3He) experiment at 80 MeV evidence has been found for a 7/2? state at 1.97 MeV in47K with a spectroscopic factor of C2S=0.08 corresponding to a ~4% admixture of πf2(s,d)?2 configurations in the ground state of Ca.  相似文献   

3.
The 48Ca(e,e′)(1+, 10.24 MeV) reaction, the 48Ca(p,p′)(1+, 10.24 MeV) reaction and the 48Ca(p,n)48Sc(1+, 16.8 MeV) reaction have been theoretically investigated with respect to the occurrence of precritical phenomena related to pion condensation. No evidence for precritical phenomena is found.  相似文献   

4.
The 48Ca(3He, 4He)47Ca and 48Ca(p, d)47Ca reactions were used to observe six levels in 47Ca above 12 MeV excitation. Analysis of the data has yielded precise excitation energies for the lowest T = 92 levels in 47Ca; which are analogs of low-lying levels in 47K. Comparison of experimental and calculated Coulomb displacement energies for the K-Ca isotopes is made.  相似文献   

5.
Absolute cross sections have been measured for the reaction 48Ca(p, γ)49Sc for 0.579 MeV ≦ Ep, lab ≦ 2.670 MeV and for the reaction 48Ca(p, n)48Sc for 0.956 MeV ≦ Ep, lab ≦ 2.670 MeV. Substantial competition effects in the cross section for 48Ca(p, γ)49Sc were observed at the thresholds for neutron emission to the 623 keV (3+), 1143 keV (2+) and 1402 keV (2?) excited states of 48Sc. Thermonuclear reaction rates were calculated from the measured cross sections for 0.1 ≦ T9 ≦ 10.0. The new rates differ considerably from those used in earlier calculations of the production of the rare, neutron-rich intermediate mass nuclides during explosive carbon burning. In particular, the new rates may change the predicted abundances for 48Ca, 49, 50Ti and 50V substantially. The good agreement between current global Hauser-Feshbach models and the experimental data indicates that Hauser-Feshbach calculations can provide sufficiently reliable rates for astrophysical calculations in cases where experimental data are non-existent.  相似文献   

6.
《Nuclear Physics A》1986,451(1):131-140
The two-proton transfer reaction (14C, 16O) has been investigated at 96 MeV on targets of 50Ti and 48Ca. The 48Ca states at 0 MeV (0+), 3.83 MeV (2+), 4.28 MeV (0+) and 4.50 MeV (3) and the 46Ar ground state were excited. The 4.28 MeV 0+state has a transfer strength comparable to the g.s. transition to 46Ar and a predominant proton vibrational character. The interpretation of the state as the proton-pairing vibrational state is supported by estimates of the excitation energy based on experimental binding energies.  相似文献   

7.
The reactions48Ca(d, t)47Ca and48Ca(3He, α)47Ca have been measured at incident energies of 17 and 18 MeV, respectively and analysed by DWBA. Besides strong transitions to the groundstate and two unresolved states at aboutE x =2.60 MeV relatively strong transitions withl=2 are observed at higher excitation energies in the (3He, α) reaction. The observedl=1 and higherl=3 transitions are rather weak indicating that particle-hole components in the48Ca groundstate are relatively small.  相似文献   

8.
The (p-d-t) process in 48Ca(p, t)48Ca(p, t)46Ca(0+, g.s.; 2+, 1.34 MeV) and 116Sn(p, t)114Sn(0+, g.s.) at 20 MeV was investigated. The calculations showed that the two-step process is important in all the transitions investigated, and is enhanced in the Sn transition by the pairing correlations in the BCS ground states.  相似文献   

9.
The yield of γ-rays from the reaction 41K(p, γ)42Ca has been measured as a function of bombarding energy over the range 0.68–2.48 MeV and from the reaction 41K(p, αγ)38Ar over the range 1.20–2.48 MeV, and the yield of neutrons from the reaction 41K(p, n)41Ca has been measured from threshold to a bombarding energy of 2.48 MeV. The energy dependence of the cross sections is compared with statistical-model calculations with global optical-model parameters in all particle channels. The calculations seriously overestimate the cross section for the neutron channel and underestimate those for the other channels. A reduction in the imaginary well depth in the neutron channel leads to good agreement with all the data. Statistical-model calculations with this modified set of parameters are then carried out to provide cross sections for the astrophysically interesting reactions 41Ca(n, p)41K, 41Ca(n, α)38Ar, and 41Ca(n, γ)42Ca. Thermonuclear reaction rates are calculated for all six reactions over the temperature range 5 × 108–1010K which includes the range of temperatures of interest in nucleosynthesis calculations.  相似文献   

10.
Excitation curves for48Ca(d, p)49Ca(0) have been measured at 12 angles in the energy region from 3.0–5.5 MeV with the aim to investigate the charge exchange effect expected at the analogous (d, n) threshold opening at 4.3 MeV. A broad flat minimum is seen in the 165° excitation curve around this threshold which is however much less significant than the charge exchange cusps observed in theA ≈ 90 mass region. More significant structure is seen atE d≈5 MeV which possibly may be connected with48Ca(4.611) core excitation or due to an intermediate state in50Sc.  相似文献   

11.
Isospin dependence of dynamical and thermodynamical properties observed in reactions 40Ca+ 40,48Ca and 40Ca + 46Ti at 25 MeV/nucleon has been studied. We used the CHIMERA multi-detector array. Strong isospin effects are seen in the isotopic distributions of light nuclei and in the competition between different reaction mechanisms in semi-central collisions. We will show also preliminary results obtained in nuclear collision 48Ca + 48Ca at 25MeV/nucleon, having very high N/Z value in the entrance channel (N/Z = 1.4). The enhancement of evaporation residue production confirms the strong role played by the N/Z degree of freedom in nuclear dynamics.  相似文献   

12.
Evaporation residue cross sections for the system36 s +48Ca were measured at Ecm=66.4 MeV, 74.4 MeV and 83.5 MeV and are compared with simple model predictions. Compound nucleus formation accounts for 80% of the total reaction cross section; the residual strength is found in the transfer channels.  相似文献   

13.
14.
The mass of 18C has been measured using the double-charge-exchange reaction 48Ca(18O, 18C)48Ti at an 18O energy of 112 MeV. The 18C ions were detected at the focal plane of a magnetic spectrometer. The mass excess of 18C was found to be 24.923 ± 0.030 MeV, and the first excited state was observed at an excitation energy of 1.62 ± 0.02 MeV. At the same time, an independent measurement of the mass excess of 17C was obtained from the 48Ca(18O, 17C)49Ti reaction, and the value 21.039 ± 0.020 MeV is in excellent agreement with an earlier measurement. The first excited state of 17C is at 295 ± 10 keV.  相似文献   

15.
《Nuclear Physics A》1986,454(1):128-142
Excitation functions have been measured for 62Ni(α, p)65Cu in the energy range 6.5–9.0 MeV, for 41K(p, α)38Ar in the range 0.8–2.6 MeV, for 41K(p, γ)42Ca, 41K(p, αγ)38Ar, 41K(p, nγ)41Ca, and 41K(p, p'γ)41 in the range 0.6–4.0 MeV, and for 41K(p, n)41Ca from threshold to 3.0 MeV. Cross sections have been extracted from the data and these are compared with statistical-model calculations based on global optical model parameters. Alternative parameter sets have been tried for the 62Ni(α, p)65Cu data and published data for 62Ni(α, γ)66Zn and 62Ni(α, n)65Zn, and both these and the global parameters have been used in statistical-model calculations of 65Cu(p, γ)66Zn, 65Cu(p, n)65Zn and 65Cu(p, α)62Ni cross sections, which are compared with published data for these reactions. Both the global and the alternative parameters lead to very good agreement with experiment for all six reactions. Alternative parameters have been tried for the 41K + p reactions also. The global parameters lead to agreement to within a factor of 2 and the alternative parameters lead to agreement to within a factor of 1.3. The 41K + p alternative parameters are used in calculations of 41Ca(n, γ)42Ca, 41Ca(n, p)41K and 41Ca(n, α)38Ar cross sections, and these and the experimental 41K + p data are used in calculations of thermonuclear reaction rates under stellar conditions for the 41Ca + n and 41K + p reactions.  相似文献   

16.
Differential cross sections for18O elastic scattering and the (18O,16C) and (18O,17N) reactions on48Ca were measured at 102 MeV using a Q3D magnetic spectrograph. The transitions to the 7/2? ground state (g.s.) of49Sc and the 0+ (g.s.), 2+ (1.554 MeV), 4+ (2.675 MeV), and 6+ (3.198 MeV) states of50Ti were analyzed by DWBA calculations which include finite-range and recoil effects. Simple cluster-transfer calculations were done for all two-proton transfer transitions. For the 0+ (g.s.) transition a two-nucleon transfer code employing microscopic wave functions was also used. It was found that absolute cross sections for this kinematically well-matched transition were underrated by a factor of about 7 for a reasonable amount of configuration mixing in the nuclear states involved in this transition. This factor is very close to the value 5 derived for the similarly well-matched48Ca(18O,16O)50Ca reaction.  相似文献   

17.
The yield of γ-rays from the reaction 42Ca(p, γ)43Sc has been measured as a function of bombarding energy over the range 0.63–3.01 MeV, from 44Ca(p, γ)45Sc over the range 0.775–4.00 MeV, from 42Ca(p, p'γ)42Ca over the range 2.24–3.01 MeV, and from 44Ca(p, p'γ)44Ca over the range 1.90–5.03 MeV. The cross section of the reaction 44Ca(p, n)44Sc has been measured from threshold to a bombarding energy of 5.05 MeV by observation of the 1157 keV γ-ray associated with the residual 44Sc activity, and the cross section of the reaction 45Sc(p, n)45Ti has been measured from threshold to a bombarding energy of 4.00 MeV both by observation of the annihilation radiation associated with the residual 45Ti activity and by measurement of the total neutron yield with a wide-angle BF3 tube and paraffin detector. All these data are compared with statisticalmodel calculations and satisfactory agreement is achieved. Thermonuclear reaction rates for the (p, γ) and (p, n) reactions are calculated for the temperature range 5 × 108-1010K and the significance of these results for explosive nucleosynthesis in stars is discussed.  相似文献   

18.
Excitation functions of the reaction39K(p, γ 0)40Ca at 0° and 90° have been taken in the proton energy range 2.5–6.0 MeV corresponding to an excitation of40Ca between 10.8 and 14.1 MeV. Positions and strengths of several resonances appearing in the excitation functions are given. The structure of40Ca is compared with predictions from 1 particle — 1 hole calculations.  相似文献   

19.
Monopole transitions from the 01+ ground states to 02+ excited states at 3.353 MeV (40Ca), 1.837 MeV (42Ca), 1.884 MeV (44Ca) and 4.272 MeV (48Ca) have been investigated with high resolution inelastic electron scattering (FWHM ≈ 30 keV) at low momentum transfer (0.29 ≦ q ≦ 0.53 fm?1). The respective monopole matrix elements are 2.53 ± 0.41 fm2, 5.24 ± 0.39 fm2, 5.45 ± 0.41 fm2 and 2.28 ± 0.49 fm2. These results are used together with known ground state charge radii and the average number of holes in the sd shell in the ground state to estimate the number of particle-hole excitations in the wave functions of the excited 0+ states.  相似文献   

20.
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