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1.
A combined analysis of the available data on the primaryγ-ray intensities from the113Cd(n, γ) reaction atE n=1.9 and 24.3 keV neutron energies together with the data on113Cd neutron capture cross sections in theE n=3–200 keV energy region was carried out. The neutron strength functions were determined asS n0=(0.260±0.073) 10?4 and Sn1=(5.06±0.67) 10?4. No spin-orbit splitting of thep-wave neutron strength function was found. The energy dependence of theE 1 radiative strength function {ie147-01} was fitted by the Kadmenski-Furman model somewhat better than by a standard Lorentzian. TheM 1 giant resonance parameters were obtained as E G M 1 =8.8±1.6 MeV and Γ G M 1 = 4.7±2.6 MeV. The neutron capture cross section of113Cd from its isomeric state ({ie147-02}=11/2?, E 1 m =263.7 keV) was calculated.  相似文献   

2.
By means of the activation technique the excitation functions for the reactions93Nb(n,2n)92mNb(10.15d),103Rh(n,2n)102mRh(2.9y), and103Rh(n,2n)102gRh(206d) were measured with an average total uncertainty of about ±8% between 10 and 20 MeV neutron energy. In addition the total93Nb(n, 2n) cross-section was compared with the59Co(n, 2n) cross-section at 16.8 MeV by direct neutron detection using the time-of-flight technique. The results are compared with statistical theory, especially with theoretical expectations for the isomeric cross-section ratios, which are only in reasonable agreement with the experiment if one assumes a ground state spinI g=5 for92Nb andI g=2 for102Rh.  相似文献   

3.
Reaction110Pd(n, 2n)109Pd has been investigated at 14.7 MeV neutrons. Cross sections for the formation of109m Pd and109g Pd were measured. Experimental value of the isomeric cross section ratio has been compared with the theoretical calculation performed with the Huizenga and Vandenbosch method.  相似文献   

4.
Isomeric cross-section ratios have been measured for the reactions107Ag(α,2n)109g,mIn and109Ag(α, 2n)111g,mIn for energies of theα-particles between 19 and 40 MeV. The experimental isomeric cross-section ratios are compared with statistical-model calculations. The program ofHafner et al. was extended by including the competition of the (α,n)- and (α, 3n)-reactions and of charged particle emission. Agreement between experiment and theory could be achieved.  相似文献   

5.
Liquid Argon was irradiated with bremsstrahlung from 18 to 31 MeV endpoint energy in steps of 2 MeV. The yields of the reactions Ar40(γ, n)+(γ, p) and Ar38(γ, n) were measured by detecting the 269a and the 35d rest activity with a low-level-counter. Cross section curves for the (γ, n)-processes could be found from the yield values, and they allowed together withσ N, σ(γ, p) andσ(γ, np) a determination ofσ(γ, 2n) and σγabs for Ar40. The integrated cross section forσ(γ, n) from threshold to 33 MeV yields (200±40) MeVmb for Ar40 and (210±40) MeVmb for Ar38, the corresponding value for σγabs being (450±60) MeVmb for Ar40.  相似文献   

6.
Proton spectra have been measured at lab angles ofθ=0° to 100° for the reaction Zr(n, p)Y at 21.8 MeV incident neutron energy. Spectra over an angular spread of 80° were accumulated simultaneously using a detection system consisting of proportional counterΔE detectors and a curved plastic scintillator as energy detector. Resonant behaviour is observed in the proton spectra for the Zr(n, p)Y reaction but not for the Fe(n, p)Mn reaction. The resonant structure is attributed to the excitation of the analogues ofT > giant dipole states of Zr. The resonant structure is shown to correspond in position, gross and fine structure, and, in strength and angular dependence of the cross sections, with expectations for the90Zr(n, p)90Y reaction. DWBA cross sections are derived and fitted to the experimental data with a Lane potential of 150 MeV.  相似文献   

7.
The induced-activity method was used to measure the isomeric ratio of the yields of the (γ, n), (n, 2n), and (γ, 2n) reactions on the 113In nucleus. The energy dependence of the isomeric ratios of the yields of the photonuclear reactions 113In(γ, n)112m,g In and 113In(γ, 2n)111m,g In is studied in the energy range of 12–35 MeV.  相似文献   

8.
Using activation techniques the cross section for the reaction27Al(n,α)24Na was determined relative to the cross section of197Au(n,2n)196Au with an accuracy of 0.3% in the energy region 13.70 to 14.42 MeV. By normalizing these data to four absolute data of other authors, the excitation function could be determined to an accuracy of 0.7%. No Ericson fluctuations could be observed, using the3H(d,n)4He as source reaction with its inherent neutron energy width.  相似文献   

9.
The isomeric ratios of the 197m,g Pt and 197m,g Hg yields in the respective (γ, n) reactions are measured for the first time in the energy range 8–17 MeV. The isomeric ratios σ mg for 197m,g Hg in the (d, 2n) reaction are measured in the energy range 8–50 MeV. The experimental data are compared with the results of theoretical calculations. The effect of the structure of low-lying states and of the yrast line on the behavior of σ mg is revealed. __________ Translated from Yadernaya Fizika, Vol. 67, No. 5, 2004, pp. 899–905. Original Russian Text Copyright ? 2004 by Zheltonozhsky, Mazur, Bigan.  相似文献   

10.
Nine experimental isomeric cross-section ratios for the reactions59Co(n, γ)60Co,60Ni(n,p)60Co, and63Cu(n,α)60Co are analysed in terms of statistical theory by means of the method ofHuizenga andVandenbosch. Theγ-cascades are treated by a new model which was recently published. The results confirm the energy dependence of the spin cut-off factor for60Coσ~U1/4 which should not be neglected. As a mean value (σ=4.3±0.3 is obtained forU=B n =7.5 MeV in good agreement with a nuclear moment of inertia for a rigid sphere.  相似文献   

11.
Absolute cross-sections and isomeric cross-section ratios have been measured for the reactions89Y(α, 3n)90g, 90m Nb. The energy of the α-particles was varied between 34 and 54 MeV. The experimental isomeric ratios are compared with statistical-model calculations.  相似文献   

12.
Activation techniques have been used to measure the cross sections at 15.1 MeV neutron energy for the following reactions: 82Se(n, 2n)81m+gSe, 81Br(n, 2n)80m+gBr, and 45Sc(n, 2n) 44m+gSc. Isomeric cross-section ratios were evaluated by applying the method of least squares to the time behavior of γ-ray activity following the ground-state decay of each isomeric pair. The absolute cross section σm for the formation of the metastable state was measured by the mixed-powder method with the 27Al(n, α)24Na reaction as the monitor. The cross section σg for the formation of the ground state was then determined by using the isomeric cross-section ratio. The sum of σm and σg for each reaction is compared with the theoretical value obtained from calculations based on the statistical model for the formation of a compound nucleus and its subsequent emission of neutrons.  相似文献   

13.
Cross sections for the reactions152Sm(n, p)152g,m1,m2 Pm,154Sm(n, p)154g,m Pm,178Hf(n, p)178m,g Lu,154Sm(n, d)153Pm and152Sm(n, α)149Nd were measured at 14.5 MeV neutron energy by the activation method. On the basis of these cross sections, the associated isomeric ratios in154Pm,152Pm,178Lu and the comparison with the predictions of different compound and precompound models, conclusions are drawn about the role of the preequilibrium processes in 14.5 MeV neutron induced reactions. Calculations for equal angular momentum removal by equilibrium and preequilibrium emitted particles better reproduced the experimental isomeric ratios, than for higher angular momentum removal in the preequilibrium phase. The isomeric ratios may be used as a source of additional information about the spin of the isomeric states in152Pm and154Pm for which the spectroscopic information is uncertain.  相似文献   

14.
The photon spectrum in the decay of164Ho was investigated using a high resolution solid state detector separating theK-X-rays of Dy, Ho and Er. The two γ-rays depopulating the 3+ and 2+ levels in164Ho were found to have energies of 56.6 and 37.3 keV. The 91.4 keV radiation of Er from our sample seems to have a non resolved high energy component with about 2.5% intensity. It may be due to the cross-over transition 3+→1+ or a sum line. The half-life of the isomeric state of164Ho was found to be 36.7 ± 1 min. The total transition rates between different levels were calculated from the measured photon intensities. The fraction 0.27 found in the branching of thee ?-capture feeding the 2+-state of Dy has nearly the same value as the analog branching in the β?-decay. Combining the measured complex ground state decay curve and the transition intensities of the isomeric and of the ground state the ground state half-live can be deduced and was found to be (28.1 ± 1.0) min. The corresponding ratio of the ground state and the isomeric state production rates is 2.84:1. A ratio of 0.04 was found for the cross section of165Ho (γ, 3n),162Ho and165Ho (γ,n)164Ho for a 90 MeV bremsspectrum.  相似文献   

15.
The cross sections for the reactions N14(n, α)B11 and N14(n, t)C12 have been measured in the neutron energy range 4.0 to 6.4 MeV and at 2.5 MeV. Mono-energetic neutrons were produced in the D(d, n) He3 reaction using a gas target. The (n, α) and (n, t) disintegrations were detected in a gridded ionization chamber filled with an argonnitrogen mixture. The response of the chamber under different operation conditions is described. The excitation functions, measured with a neutron energy resolution of 40 to 50 keV, are given for theα 0 group from the N14(n,α)B11 reaction over the entire neutron energy range and for theα 1 group and the t0 group from N14(n, t) C12 for neutron energies above 4.3 and 5.6 MeV, respectively.  相似文献   

16.
R K Jain  H S Virk  J Rama Rao  S K Bose 《Pramana》1997,49(5):515-519
Fission-track registration characteristics of Lexan solid state nuclear track detectors have been used to measure the fast neutron induced fission cross section of232Th. The fast neutrons (?14.2MeV) were produced with the help of an AN-400 model Van-de-Graaff accelerator at Banaras Hindu University laboratory using3H(2H,n)4He reaction and were used to irradiate the fissile target deposited on the plastic detector. The track densityT, registered on the plastic detector is related to the fission cross sectionσ f, through the relationT=knσ føt wheren is the number of fissile atoms per cm2 in the deposit, ø is the neutron flux,k is fission track registration efficiency andt is the time of irradiation. The fission cross sectionσ f of232Th, relative to the well measured fission cross section of238U, was found to be 0.36±0.04 barn.  相似文献   

17.
The cross-sections for formation of isomeric pair, 75Gem(σm) and 75Geg(σg), through 76Ge(n, 2n), 75As(n, p) and 78Se(n, α) reactions were measured at 13.73 MeV, 14.42 MeV and 14.77 MeV neutrons and also estimated using EMPIRE-II and TALYS codes over neutron energies from near threshold to 20 MeV. For each (n, 2n), (n, p) and (n, α) reaction, the cross-section initially increases with neutron energy, but starts decreasing as the neutron energy exceeds the respective threshold of (n, 3n), (n, pn) and (n, αn) reactions. The higher values of σm relative to σg reveal that the transitions of the excited 75Ge from higher energy levels to metastable state (7+/2) are favored as compared to unstable ground state (1/2). The present values of cross sections for formation of 75Gem,g through (n, 2n) and (n, α) reactions are lower, and that of (n, p) reaction are higher compared to most of the corresponding literature cross-sections.  相似文献   

18.
Cross sections for the reactions27Al(n, p)27Mg and28Si(n,p)28Al were measured by activation method between 13.40 and 14.83 MeV neutron energy. An accuracy of about 4% was achieved using the27Al(n, α)24Na reaction as a reference at 14.1 MeV where the relative excitation function has also been measured. Results obtained were compared to a recent compilation and that calculated by the Hauser-Feshbach model. Using the back-shifted level density formula and taking into account the contribution of the separated levels, the calculations were extended to the energy range from the threshold to 18 MeV. A structure was observed in the27Al(n, α)24Na reaction cross section curve around 14 MeV neutron energy.  相似文献   

19.
In order to obtain data on the photon absorption process between the giant resonance and the meson threshold the cross sections of the reactions12C(γ,n)11C,12C(γ, 2n)10C,39K(γ,n)38Kg, and40Ca(γ,np)38Kg have been determined by the analysis of yield curves at the 140 MeV electron synchrotron of the PTB. Though the (γ,n) cross sections grow small with increasing photon energy they are different from zero up to energies of 60 MeV and above. The cross section of the reaction12C(γ, 2n) is extremely small; its highest value amounts to 0.15% of the highest value of the12C(γ,n) reaction. The measured40Ca(γ,np) cross section is of the order predicted by the naive quasi-deuteron model. The integrated cross sections of the above reactions up to 140MeV are 85±7,0.90±0.10, 139±16, and 76±7MeVmb respectively.  相似文献   

20.
Previously measured angular distributions of the differential cross section and the tensor analyzing powerT 20 for the scattering of7Li from51V in the energy range from 10 to 18 MeV were analyzed with the double folding model using the effective nucleon-nucleon interaction M3Y as well as a zero range effective nucleon-nucleon interaction. Due to the spectroscopic deformation of the7Li-nucleus the interaction potential contains a central and aT R -tensor part. The latter one is the origin of the observed tensor analyzing powers. Within the same model the scattering of aligned7Li-nuclei from58Ni at 14.2 and 20.3 MeV is well described. The strength of theT R -tensor potential in relation to the spectroscopic mass deformation of7Li is discussed. Using the real interaction potential obtained by the double folding model the energy dependence of the total reaction cross sectionσ r and its tensor analyzing powerT 20 r for the system7Li?51V is well described within a barrier penetration model.  相似文献   

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