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1.
The sub-Coulomb (t,α) reaction has been employed in the determination of the rms radii of the 3s12, 2d32, 1h112, and 2d52 proton orbits in 208Pb. The experimental values are compared to the results of Hartree-Fock calculations.  相似文献   

2.
A shell-model calculation of the N = 51, 39 ≦ Z ≦ 42 nuclei is presented. The 88Sr nucleus is assumed to be an inert closed core. The extra-core protons are restricted to the (2p12, 1g92) configurations, and the active neutron is allowed to occupy the 2d52, 3s12, 2d32 and 1g72 orbits. The proton-proton effective interaction is directly taken from the previous analysis on the energy levels for N = 50 isotones by Ball et al. The proton-neutron effective interaction is assumed to be of the form of the surface δ-interaction. The energy spectra are calculated from a least-squares fit to the experimental data, varying the T = 0 and T = 1 strengths of the surface δ-interaction. Spectroscopic factors, E2 transition rates and two-body matrix elements are also calculated and compared with the observed values and the previous theoretical results.  相似文献   

3.
The results of high-resolution studies of the 91Zr(d, p) reaction at Ed = 12 MeV and the 90Zr(t, p) reaction at Et = 11.85 MeV are presented. Absolute cross sections have been measured for both reactions and (d, p) spectroscopic factors determined. A comparison of these results with earlier data has been made, and although many of the previous assignments have been confirmed, many new features concerning the structure of 92Zr have been discovered. Shell-model calculations have been performed for 91Zr and 92Zr using a neutron space which includes the 2d52, 3s12, 2d32, 1g72 and 1h112 orbits and a proton space comprising the 1g92 and 2p12 orbits. Realistic proton-neutron and neutron-neutron interactions based on the Sussex matrix elements were used in the calculations. Spectroscopic factors have been calculated for the 90Zr(d, p) and 91Zr(d, p) reactions and cross sections calculated for the 90Zr(t, p) reaction. In general, good agreement between the theoretical and the experimental results has been obtained.  相似文献   

4.
Sub-Coulomb (t, α) reactions have been employed in the determination of the rms radii of the 1g92, 2p12 and 2p32 proton orbits in 112,116,118,120,124Sn. The experimental values are compared to the results of Hartree-Fock calculations.  相似文献   

5.
An optimized Woods-Saxon potential, which gives excellent fits to the observed proton states in 209Bi and 207Tl, is used to calculate the excitation energy of the unbound 3p12 proton state in 209Bi. Using the wave functions given by the above potential, the strength of the core-particle interaction is calculated. The effect of the vibration of the core on the fragmentation of the 3p12 state is estimated. It is found that the 3p12 state at 5.123 MeV loses more than 80% of its strength to five 12? collective states in 209Bi and the observed 3p12 state at 3.64 MeV is actually an almost equal mixture of the 3p12 single-proton state and the (4+, 1h92) collective state.  相似文献   

6.
The excitation functions of 208Pb(p, p0)208Pb have been measured in the energy range Ep = 14.2 to 17.4 MeV in 50 keV steps at θlab = 120°, 140° and 160°. The isobaric analog resonances of the parent states in 209Pb up to Ex = 2.5 MeV and the optical-model background were fit simultaneously at all energies and angles. The spreading widths and the values of a parameter β2, which measures the isospin purity of the IAR, were determined for the g92, i112, j152, d52, and s12 resonances. An average value of the isospin purity of β2 = 66% was found.  相似文献   

7.
The collective bands of states of 68Ge are studied using a deformed-configuration-mixing shell model based on Hartree-Fock intrinsic states. An effective interaction given by Kuo has been used. The configuration space includes the single-particle orbits 1p32, 0f52, 1p12and 0g92. The collective positive- and negative-parity states are classified into different bands on the basis of the E2 transition probabilities amongst them. The agreement with the experiment is quite satisfactory. An attempt has been made to understand the structure of the nearly degenerate triplet of the 8+ states and their decay schemes.  相似文献   

8.
9.
The 41Ca(d, p)42Ca reaction has been used to locate the strength distributions for p32 and p12 transfer in 42Ca. Effective (f72)2, f72p32 and 7212 two-body matrix elements are derived from the data and compared to theoretical predictions.  相似文献   

10.
In this note we determine the oscillator strengths for the dipole absorption of neutral bound excitons in direct gap semiconductors, using our previously obtained 35-term Page and Fraser type wave function, and taking into account the detailed electronic structure as well as the electron-hole exchange interaction.The envelope part of the oscillator strengths varies considerably with the electron-hole mass ratio σ = m1em1h, and is maximum for the (D0, X)- complex when σ = 0.4. For typical σ-values (σ? 0.1–0.2), ?(D0,X) ? 10?(A0,X). But when σ approaches zero, the overlapping of the electron and the hole envelope wave functions of the (A0,X)-complex decreases progressively so that the oscillator strength also decreases and tends to zero.In the case of zinc-blende materials (Td) and positive spin-orbit coupling at k = 0, we confirm that the line strength for transitions to or from J = 126) or J = 527 + Γ8) level of the (A0, X)-complex is equal to one quarter of the line strength to or from the J = 328) level.In the case of CdS, where our computed values are only in qualitative agreement with the experimental values, we discuss the use of the phenomenological result of Rashba.  相似文献   

11.
12.
Cross sections for charmed baryon pair production near threshold in e+e? annihilation are calculated using pole-dominated form factors modified to take intoccount continuum effects. When the C0+C0? production cross section is normalized with the help of data for e+e?pX it is found that the total charmed baryon production cross (C0C0, C1C1, C1C11 + C11C1, C11C11) reaches a peak value of approximately 2.7 nb at √s = 5 GeV.  相似文献   

13.
We present a multilevel calculation within the framework of the interacting boson-fermion model (IBFM-1) of the odd-mass 101–109Rh isotopes. We calculate both positive- and negative-parity states of the same hamiltonian, starting from the 1g92, 2p12, 2p32, lf52 and 2d52 single-particle orbitals. We discuss energy spectra, electromagnetic E2 transition rates and one-nucleon transfer properties. We also discuss the influence of the 1f72 orbital on the one-nucleon transfer properties. The results of the calculation for the negative-parity states are compared with the results of the U(612) supersymmetry scheme of the interacting boson model.  相似文献   

14.
15.
Differential cross sections were measured for 46Ti(p, p) and 46Ti(p, p1) at four angles between Ep = 1.5 and 3.1 MeV, with an overall energy resolution of about 300 eV. Spins, parities, total and partial widths were extracted for 144 resonances. Six analogue states were identified. The s-wave states have expected spacing and width distributions, while the p12 states behave anomalously. The s12, p12 and p32 strength functions were determined.  相似文献   

16.
The results of a vibrational and rotational analysis of the banded a?3A2X?1A1 transition in CH2SCD2S are presented. Only three of the six vibrational modes are active in the spectrum with ν′2 = 13201012, ν′3 = 859798, and 2ν′4 = 711516cm?1. The spin forbidden transition gains intensity primarily by a mixing of the 1A11,π) and 3A21,n) states. This is confirmed by a rotational analysis of the 000 band of both isotopes. The rotational analysis shows that the coupling in the a?3A2 state is near Hund's case b and that the spin constants are nearly 10 times greater than those observed for CH2O. A CNDO2 calculation shows that this difference is due to the greater spin orbit coupling of S in CH2S and to the smaller energy differences between the B?1A11,π), b?3A11,π), X?1A1, and the a?3A21,n) states. The r0 structure calculated from the rotational constants is rCS = 1.683 A?, rCH = 1.082 A?, βHCH = 119.6°, and α (out of plane) = 16.0°. A simultaneous fit of the vibrational levels in ν4 of CH2S and CD2S to a double minimum potential function yielded a barrier to molecular inversion of 13 cm?1 and an equilibrium out-of-plane angle of 15°.  相似文献   

17.
From a study of (p,t) reactions on 31P and 30Si it is suggested that in 29P the states with Jπ=121+ and 122+, the pair 322+, 521+, and the pair 723+, 921+ are related by weak coupling of a s12 proton with the states 01+, 02+, 21+ and 41+ respectively of 28Si. Completely atypical L = 2 angular distributions have been obtained for the 321+ and 522+ states in 29P and it is suggested that this is due to contribution by two-step processes.  相似文献   

18.
The method of multiple scales is used to analyze the response of a single-degree-of-freedom system to either the combination resonance of the additive type Ω2 + Ω1 ≈ ω0 or the combination resonance of the difference type Ω2 ? Ω1 ≈ ω0, where Ω1 and Ω2 are the frequencies of the excitation and ω0 is the linear undamped natural frequency of the system. To the second approximation, the combination resonance of the additive type has three effects on the steady state response. First, it produces terms having the frequencies Ω1, Ω2 and Ω2 + Ω1 at first order and terms having the frequencies 0, 1, 2Ω2, Ω2 ? Ω1, 2(Ω2 + Ω1), Ω2 + 2Ω1 and 2 + Ω1 at second order. Second, it produces a shift in the natural frequency of the system. Third, it produces a virtual primary-resonant excitation having the frequency Ω2 + Ω1 ≈ ω0 that makes the component having the frequency Ω2 + Ω1 be of first rather than second order. Similar effects are produced by a combination resonance of the difference type or a superharmonic resonance of order two.  相似文献   

19.
Accurate SCF computations are reported on the Rydberg states of N2 of electron configurations ---1πu3u, ---1πu3u, and ---3σg2πg, also on the valence states of the configuration ---1πu3g. The Rydberg state calculations supplement those of Lefebvre-Brion and Moser. A comparison is made between the ---1πu3u states and the parallel set of states of the u3g configuration. This comparison shows a sharp difference in the 1Σ+ states of the two configurations, the 1Σ+ state being very high in the latter but relatively low in the former configuration. Recknagel coefficients are given for the several states of the two configurations; as expected, these are much smaller for the u3u configuration. Also, the 1Δ state is relatively lower for the latter configuration.  相似文献   

20.
Hyperfine structure of the (0, 0, 1) - (1, 0, 1) transition of methanol has been investigated by beam absorption and of the (J, 1, 3?) → (J, 1, 3+) transitions for J = 2, 3, and 6 by beam-maser spectroscopy. The best-fit results for the spin-rotation and spin-spin coupling constants CJKτ±(i) and DJKτ±(i), respectively, are in kHz1: C101(1) = 2.4(10), C101(2) = ?0.6(10), D101(1) = ?13.8(9), D101(2) = 7.0(9), C213?(1) = ?5.0(10), C213?(2) = ?5.5(10) and (CJ13?(2) - CJ13+(2)) = 0.98(9).  相似文献   

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