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Results

GNEIS RESULTS

Russian version
Investigations of the (n,gf)-reaction in neutron resonances of 235U and 239Pu.
Study of the neutron capture reaction for 238U.
Measurement of the forward-backward asymmetry in slow neutron fission.
Measurement of the neutron total cross sections of 209Bi and 208Pb: estimate of the electric polarizability of the neutron.
Estimation of the neutron polarizability from joint analysis of the total cross-sections of lead-208 and carbon.
Measurements of the neutron total cross sections of lead isotopes.
Study of the fast neutron induced fission of 233U, 238U, 232Th, 237Np and 239Pu in the energy range up to 200 MeV.
Study of the fast neutron induced fission of lead and bismuth in the energy range up to 200 MeV.
Study of the fission neutron multiplicity for spontaneous fission of 244Cm, 248Cm and 252Cf.

Investigations of the (n,gf)-reaction
in neutron resonances of 235U and 239Pu.

O.A. Shcherbakov, A.B. Laptev, G.A. Petrov
     Experimental studies on the two-step (n,gf)-reaction give unique information not only about fission process itself, but also about the structure of highly excited states in heavy nuclei, both in 1-st and 2-nd wells of the fission barrier, and radiative transitions between them. The fission g-ray multiplicity has been measured in neutron resonances of 235U and 239Pu. The experimental prefission widths Ggf have been obtained from the observed correlations between the multiplicity of fission g-rays and reciprocal fission width Gf-1 of resonances:
235U: Ggf (4-) = 0.32 meV  ±  0.13 meV
Ggf (3-) = 0.87 meV  ±  0.89 meV
239Pu: Ggf (1+) = 1.9 meV ± 0.8 meV
Ggf (0+) = 2.8 meV ± 9.2 meV

     The experimental and calculated prefission width Ggf is shown in Fig. 1 for the 4--resonances of 235U and 1+-resonances of 239Pu as function of the ratio of the E1 and M1 components in the prefission g-ray spectrum. The comparison of the experimental and calculated Ggf-widths shows predominance of the M1 radiation in compound nucleus 236U and that of E1 radiation in the prefission spectra of g-transitions between the highly excited states in compound nucleus 240Pu. It was also found that the best agreement between experiment and calculations is obtained by using the model of intermediate damping of the vibrational states in the second well and the Giant Dipole Resonance model.

Results of GNEIS, Fig.1
Fig. 1. Experimental and calculated widths Ggf for 1+-resonances of 239Pu and 4--resonances of 235U. Calculation model: I - single-humped fission barrier, II, III - double-humped barrier (complete and intermediate damping of the vibrational states in the second well, respectively); a - single-particle model (Weisskopf) for probabilities of g-transitions; b, c - GDR model (Axel-Brink, Lorentzian-shaped probability of partial g-transitions proportional to Eg4 and Eg5, respectively).
     In another experiment at the GNEIS, the pulse-height spectra of fission gamma-rays have been measured in isolated resonances of 239Pu in the energy range from 10 eV to 91 eV. The difference pulse-height spectra for weak (Gf < 10 meV) and strong (Gf > 10 meV) 1+-resonances show a few structures that could be interpreted as prefission gamma-transitions between the levels at excitation energy 1 - 3 MeV below the neutron binding energy Bn.
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Measurements of the capture cross-section of 238U
in energy range En<100 keV and gamma-ray spectra from
the capture of resonanse neutrons: study of the nature
of the 721.6 eV resonance.

O.A. Shcherbakov, A.B. Laptev
     Two lowest energy resonance clusters in the subthreshold fission cross-section of 238U are dominated by the 721.6 eV and 1211.4 eV resonances. Anomalously small capture width of the 721.6 eV resonance (~ 4.7 meV) is a strong evidence that this resonance is not usual (class-I, corresponding the first well of fission barrier) compound state. If the 721.6 eV resonance is predominantly class-II (corresponding to the second well) in character, then not only its radiative width Gg should be small, but the capture g-ray spectrum of this resonance should be softer than that of other s-wave resonances (class-I). Prior to present measurements, J.C. Browne (1976) observed a much softer g-ray spectrum for the 721.6 eV resonance than for neighboring resonances, whereas H. Weigmann et al. (1975) found no difference. To resolve this contradiction, the capture g-ray spectra in isolated neutron resonances of 238U in the energy range from 400 eV to 1300 eV have been measured at the GNEIS. The data obtained have been processed after the slightly modified method of Weigmann et al. The idea was to detect a g-decay branch within the second well using two different bias values for the g-ray registration: lower B1 and upper B2. Then, for value of B2 larger than Bn- EII (2 MeV, height of the second minimum), the ratio of resonance area Ag measured with two biases B1 and B2:
R = Ag(bias B2)/Ag(bias B1)

should be smaller for the resonance having major class-II fraction than for ordinary class-I resonances because the softer class-II component will be under the upper bias B2 for this resonance.
     The results of the present measurements and those of Weigmann et al (Geel) are shown in Fig. 2. As it is seen from our data, the capture g-ray spectrum of the 721.6 eV resonance is much softer than that of the neighboring s-wave resonances. Our data enable to make a conclusion that the 721.6 eV resonance is predominantly class-II by nature. As for the 1211.4 eV resonance, both our data and the results of Weigmann et al show that there are no solid arguments to consider this resonance as a class-II state.

Results of GNEIS, Fig.2

Fig. 2. Results of the capture g-ray measurements for resonances of 238U.
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Measurement of the forward-backward asymmetry in slow neutron fission.

V.E. Sokolov, A.M. Gagarsky, A.B. Laptev, A.K. Petukhov, G.A. Petrov, O.A. Shcherbakov
     Parameters and decay properties of low energy p-resonances in heavy fissile nuclei are practically unknown because of the difficulties existing when generally accepted method are used. The new method to obtain such information is the study of the neutron energy dependence of the forward-backward asymmetry of angular distribution of fission fragments which is the result of s- and p-wave interference in neutron capture

W(Q) = 1 + afb·(pn·pf)

where pn and pf are the neutron and light fragment momenta. The principal advantage of this method if compared with the other asymmetry-measurements: a non-polarized neutron beam can be used. The measurements of the forward-backward asymmetry coefficient afb for 235U and 233U from 1 eV to 136 eV have been performed at the GNEIS. The results obtained for 235U in the energy range from 1 eV to 21 eV are shown in Fig. 3.

Results of GNEIS, Fig.3

Fig. 3. Energy dependence of the asymmetry coefficient afb and fission yield for 235U.
     Several irregularities caused by p-resonances have been observed in energy dependence of the coefficient afb. Estimations of the main p-resonance parameters have been made. Fitting analysis of the data gives that the average total width of the p-resonances is some greater than that of s-resonances. For example in case of 235U <Gfp> = (200 ± 50) meV and <Gfs> = (140 ± 10) meV. On the base of analysis of this data, the evaluation of fast direct fission (without compound nucleus stage) contribution to the total fission cross section was obtained. It was found to be lower than 5·10-2 at 95 % - level of reliability.
     The information obtained in these measurements is very important for the fundamental investigations of the P- and T-parity violation effects that are expected to be resonancely enhanced in a vicinity of p-resonances.
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Measurement of the neutron total cross sections of 209Bi and 208Pb:
estimate of the electric polarizability of the neutron.

A.B. Laptev, I.S. Guseva, G.A. Petrov, O.A. Shcherbakov, Yu.A. Alexandrov, V.G. Nikolenko
     The electric polarizability an is one of the characteristics of the neutron as an elementary particle and determines the induced electric dipole moment in an external electric field: D = anE. It is known [1] that information about polarizability of the neutron can be obtained from the neutron total cross section measurements for heavy nuclei. In Coulomb field, an addendum

V = - 1/2·DE = - 1/2·an Z2 e2 /r4

caused by polarizability is added to the neutron-nucleus interaction potential, which in total scattering cross section leads to several additional terms, main of them sp linear depended on k, where k is the wave number (or, the same, on sqrt(En) , here En is neutron energy). The contribution of sp to the total cross section of heavy nuclei such as 209Bi or 208Pb approximately can be written as

sp» 10-4·an·sqrt(En)  barn .

Here an is in 10-3 fm3 units and En is in eV. So far as with an increase of neutron energy, a contribution of this term in total cross section increases in proportion to the wave number k, then, from the principal standpoint, a measurement of polarizability could be reduced to comparison of total cross sections measured at different energies. To date, several attempts have been performed to measure of an , for references see [2].
     The total cross-section of 209Bi in the energy range from 1 eV to 100 eV and that of 208Pb from 1eV to 20 keV have been measured at the GNEIS facility for the purpose of estimating a value of an . Simultaneously, the total cross section measurements for silicon and carbon were carried out as a zero-test of the experiment. For silicon and carbon, the polarizability influence should be negligibly small in comparison with that of bismuth and 208Pb because the polarizability contribution to the cross section is proportional to the square of nuclear charge Z2.
     The 40-m flight path was used. The ionization 3He-chamber was used as neutron detector. Resonance filters of Co(132 eV, 4.3 keV, 5.0 keV), W(18.8 and 4.16 eV), In(1.46 eV) and Al(34 keV) were placed in the beam for permanent background monitoring. In order to suppress the overlap neutrons, cadmium filter was placed in the beam. For a distortion of the spectrum shape caused by nonzero dead time to be equal for bismuth-silicon and 208Pb-carbon pairs, the samples thicknesses were chosen for their transmissions to be about equal in energy range of interest.
     The measured total cross sections of 209Bi and Si are shown in Fig. 4 and that of 208Pb and C in Fig. 5. The given errors are statistical ones and reflect uncertainties of cross section energy dependence. Only the energy dependence of cross section is used for an-value estimation. In order to evaluate a value of polarizability it is necessary to subtract from total cross section the corrections for Schwinger and (n,e)-interactions, solid state correction, absorption cross section and neutron resonances contribution.

Results of GNEIS, Fig.4 Results of GNEIS, Fig.5
Fig. 4. Measured total cross sections of 209Bi and Si.
Fig. 5. Measured total cross sections of 208Pb and C.

Bismuth
     Analysis of the data for Bi using the method given in [3] with simultaneous variation of two parameters - polarizability and resonances contribution (parameter P2 from [3] ) - leads to an = (25 ± 11)·10-3 fm3. One can not obtain better precision of an for Bi data because of the large contribution of 800 eV resonance.
Lead-208
     Applied method of evaluation of an-value for 208Pb is described in detail in ref. [4]. In accordance with [4] total cross section of 208Pb for investigated energy range can be written under two very common assumptions - optical theorem and first Born approximation - as:

st/4p = (1/4·S2 + 1/4·S3 - 1/2k2 ) cos(2d0 + 2h0 + 2z0) -
- 1/2k ·S1·sin(2d0 + 2h0 + 2z0) + 1/2k2 ·cos(2h0 + 2z0) .

Here (d0 + h0 + z0) is sum phase of s-scattering:
    d0 = - k R0'- describes pure nuclear interaction (R0'- radius of potential s-scattering),
    h0 = k ane F - due to (n,e)-interaction (F - integrated electron form-factor),
    z0 = fa k (6/5 - p/3 ·kR - 5/7 ·(kR)2 ) - additional part of phase of s-scattering caused by neutron polarizability, fa = man/R ·(Ze/h)2R - radius of nucleus.
Terms S1, S2 and S3 are due to resonances. Thus, there are three parameters -R0', ane and an- for least square fitting procedure in our energy range. Accuracy of an estimation is strongly dependent on the number of fitting parameters. And in case of 208Pb an estimated value of the neutron electric polarizability is found to be an = (2.4 ± 1.1)·10-3 fm3.
     In our opinion, the estimated value of an is in agreement with zero value. A further progress in increasing the precision of an-measurements could be related with the substitution of neutron detector for more effective one and in conjunction with detailed background analysis and therefore increasing the high-energy boundary of measured cross section. That leads to an increase of polarizability contribution to the total cross section because it depends on energy as sqrt(En) .
     Especially, we would like to say about a nonzero value obtained at Oak Ridge [5] for neutron polarizability an = (1.20±0.15±0.20)·10-3 fm3. We think that Oak Ridge value of an does not close the problem of neutron polarizability. Analysis of method of an-value evaluation in ref.[5] allows to make several conclusions [4]:
1. Radius of potential s-scattering R0' evaluation in ref. [5] was made for total cross section by means of code REFIT without taking into account contributions due to an and (n,e)-interactions. But both of them interfere with potential interaction. Thus, R0' was in fact struck off varied parameters and that must strongly underestimate an error. An analysis of our data showed strong correlation between R0' and an [2].
2. The use of cross-section parametrization [5]

s(k) = s0 + s1 k + s2 k2 + O(k4)
is correct if simplification
sin d0» d0
is right (up to several keV). But in fact, the data up to 40 keV were involved into analysis.
3. It is necessary to take into account p-wave component of potential scattering in total cross-section analysis at neutron energy above 20 keV because at that energy value of p-wave contribution becomes comparable with that of an for expected value of neutron polarizability. For correct analysis of data [5] at energy above 20 keV, the additional fitting parameter R1' should be used, but that will increase error of an-estimation.
     Thus, we think that error of an-value estimation in ref. [5] is very underestimated and the problem of neutron electric polarizability measurement deserves further research.
     Final part of this work was supported by RFBR Grant # 97-02-16184.
References
1. Yu.A. Alexandrov, Yadern. Fiz. 37, 253 (1983); 38, 1100 (1983).
2. Yu.A. Alexandrov, I.S. Guseva, A.B. Laptev, V.G. Nikolenko, G.A. Petrov, O.A. Shcherbakov. In book "V International Seminar on Interaction of Neutrons with Nuclei "Neutron Spectroscopy, Nuclear Structure, Related Topics", ISINN-5, Dubna, May 14-17, 1997". Dubna, JINR, E3-97-213, 1997, p. 255-260.
3. Yu.A. Alexandrov, M. Vrana, J. Manrique Garcia, T.A. Machekhina and L.N. Sedlakova, Yadern. Fiz. 44, 1384(1986).
4. I.S. Guseva, PNPI Preprint 1969, Gatchina, 1994.
5. J. Schmiedmayer, P. Riehs, J.A. Harvey, N.W. Hill, Phys. Rev. Lett. 66, 1015 (1991).
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Estimation of the neutron polarizability
from joint analysis of the total cross-sections of lead-208 and carbon.

A.B. Laptev, I.S. Guseva, G.A. Petrov, O.A. Shcherbakov
     It is well known [1] that information about polarizability of the neutron can be obtained from the neutron total cross section measurements for heavy nuclei. To date, a lot of the neutron total cross section measurements for heavy nuclei have been performed to evaluate an [2]. Investigators approach closely the upper limit of polarizability about 1·10-3 fm3. The sole exception is the result [3] an = (1.20±0.15±0.20)·10-3 fm3 obtained in Oak Ridge. But in spite of a nonzero value of an , most investigators [4,5,6] think that error of this result [3] is very underestimated because it takes no account of additional parameters necessary to fit the total cross section with the aim to evaluate an.
     In that situation, when investigations achieved very small error for an-value, it is clearly to understand the importance of taking into account of all circumstances that can to lead to distortion of total cross section. In our previous work [2] the main problem caused an anxiety was systematical errors of total cross sections because of errors in knowing of experimental background value (see chapter "Measurement of the neutron total cross sections of 209Bi and 208Pb: estimate of the electric polarizability of the neutron" in this page). In this work the neutron total cross sections has been measured with an accuracy Ds/s ~ 10-3 for 208Pb and C in the energy range from 1 eV to 20 keV using the time-of-flight facility GNEIS in Gatchina. The results of the total cross section measurements for 208Pb and C are shown in Fig. 5.
     The method employed for evaluation of an for 208Pb is described in ref. [4]. Fitting results for 208Pb are presented in Fig. 6. Points are experimental total cross section after the Schwinger and solid-state corrections and contribution of radiative absorption having been subtracted. The reduced c2 is equal 2.5 for this fitting. The neutron polarizability obtained is an= (2.4 ± 1.1)·10-3 fm3 and the amplitude of neutron-electron interaction is ane = - (1.78 ± 0.25)·10-3 fm .
     Fitting results for carbon are presented in Fig. 7, the value of reduced c2 is equal 1.7 . From Figures 6 and 7 we can see that group of points in vicinity of energy about 1 keV lies systematically higher than fitting curve. This energy region corresponds to the case when the experimental background changes sharply its energy behaviour. Therefore, the experimental background at this energy range can not be satisfactory described using conventional resonance filter method.
     The total cross section measurements for 208Pb and C were carried out in similar experimental conditions [2]. At the same time, the samples thicknesses were chosen for their transmissions to be about equal in energy range of interest. As the result, the experimental background were equal in cases of 208Pb and C in these measurements and, therefore, distortions caused by uncertainties of experimental background should influence on the measured total cross sections of 208Pb and C in the same manner. Thus, to eliminate influence of the distortions caused by uncertainties of experimental background, the difference

s(208Pb) - const ·—s(C)

has been used for the neutron polarizability estimation. Here a value of const = 2.42 was chosen, so that the average value of the difference to be about equal to zero in the energy range under investigation. Fitting results for this difference are shown in Fig. 8. Using this method, the polarizability was obtained near the same value an = (2.44 ± 1.32)·10-3 fm3 . The value obtained for amplitude of neutron-electron interaction is ane = - (1.75 ± 0.27)·10-3 fm , the value of reduced c2 is equal 0.7 .

Results of GNEIS, Fig.6
Results of GNEIS, Fig.7
Fig. 6. Fitting results for 208Pb.
Fig. 7. Fitting results for C.
Results of GNEIS, Fig.8
Fig. 8. Fitting results for difference s(208Pb) - 2.42·—s(C).

     This method of joint analysis of the experimental data is very useful in the way of obtained sure result for an independent on experimental background. That is very important in case of experimentalists achieve level of precision when systematical errors of measured cross section due to experimental background are compare with statistical one. In our opinion, the estimated value of an is in agreement with zero value at present time and the problem of neutron electric polarizability measurement deserves further research.
     This work was supported by RFBR Grant # 97-02-16184.
References
1. Yu.A. Alexandrov, Yadern. Fiz. 37, 253 (1983); 38, 1100 (1983).
2. Yu.A. Alexandrov, I.S. Guseva, A.B. Laptev, V.G. Nikolenko, G.A. Petrov, O.A. Shcherbakov. In book "V International Seminar on Interaction of Neutrons with Nuclei "Neutron Spectroscopy, Nuclear Structure, Related Topics", ISINN-5, Dubna, May 14-17, 1997". Dubna, JINR, E3-97-213, 1997, p. 255-260.
3. J. Schmiedmayer, P. Riehs, J.A. Harvey, N.W. Hill, Phys. Rev. Lett. 66, 1015 (1991).
4. I.S. Guseva, PNPI Preprint 1969, Gatchina, 1994.
5. V.G.Nikolenko, A.B.Popov, Preprint JINR E3-92-254, Dubna, 1992.
6. T.L.Enik et al. In book "IV International Seminar on Interaction of Neutrons with Nuclei "Neutron Spectroscopy, Nuclear Structure, Related Topics", ISINN-4, Dubna, April 27-30, 1996". Dubna, JINR, E3-96-336, 1996, p. 205.
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Neutron Total Cross Sections of 204Pb, 206Pb, 207Pb and 208Pb.

A.B. Laptev, I.S. Guseva, G.A. Petrov, O.A. Shcherbakov, I.L. Karpihin, P.A. Krupchitsky
     The neutron total cross sections have been measured for lead isotopes 206Pb, 207Pb and 208Pb in the range from 1 eV to 20 keV and for 204Pb (preliminary results) in the range from 1 eV to 100 eV using the time-of-flight facility GNEIS. The main experiment devoted to measurement with 208Pb was carried out with the aim to measure a value of electric polarizability of the neutron (see previous experiment). Measurements with 204Pb, 206Pb and 207Pb were carried out with the aim to obtain  more exact corrections to be taken into account for other lead isotope admixtures in neutron total cross section of 208Pb. Additional motivation of these measurements is that numerical data on neutron total cross sections of lead isotopes are scarce and at low energies -  practically absent (for example see EXFOR, IAEA-NDS-CD-05, EXFOR on CD-ROM, Version 21 January 2000 and CINDA on CD-ROM, Version December 1999, Rev.1, NEA Data Bank, Paris). The following samples were used for present measurements: a 5.14-g sample of 204Pb with isotopic composition 204Pb - 36.6%, 206Pb - 30.6%, 207Pb - 13.2%, 208Pb- 19.6%; a 110.2-g sample of 206Pb with isotope composition 206Pb- 91.2%, 207Pb - 6.0%, 208Pb - 2.8%; a 106.7-g sample of 207Pb with isotope composition: 204Pb < 0.04%, 206Pb - 4.04%, 207Pb - 84.4%, 208Pb - 11.56%; and 231.6-g sample of 208Pb with isotope composition: 206Pb - 1.08%, 207Pb - 1.79%, 208Pb - 97.12%.
     The total cross section measurements were performed using a conventional transmission method. Experimental arrangement was placed on a 42-m flight path. The ionization 3He-chamber was used as neutron detector and it was housed in a composite shielding. The "black" resonance filters of Al (34 keV), Co (5.0 keV, 4.3 keV, 132 eV), W (18.8 and 4.16 eV) or Ta (4.28 eV), In (1.46 eV) and Cd (0.3 eV) were placed in the beam for permanent background monitoring. To compensate for neutrons flux fluctuations, the "sample in beam" and "sample out of beam" measurements were carried out in short (10 min.) runs in case of 206Pb, 207Pb and 208Pb. An accuracy of the measured neutron total cross section is about Ds/s ~ 5·10-2 for 204Pb, Ds/s ~ 10-2 for 206Pb and 207Pb, Ds/s ~ 10-3 for 208Pb.
     This work was supported by RFBR Grants # 97-02-16184  and  00-02-17876.
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Neutron induced fission cross-sections of 233U, 238U, 232Th,
237Np and 239Pu relative to 235U from 1 MeV to 200 MeV.

O.A. Shcherbakov, A.B. Laptev, G.A. Petrov, A.S. Vorobyev, A.Yu. Donets, A.V. Evdokimov, A.V. Fomichev, T. Fukahori, V.M. Maslov, Yu.V. Tuboltsev
     There is a long standing need in information about fission of heavy nuclei induced by the particles at intermediate energies. Regular experimental studies of fission in this energy region started comparatively recently, mainly due to the increased capabilities of modern neutron sources and experimental techniques. Among new applications of the fission data above 20 MeV, the most important are accelerator-driven transmutation of waste reactor materials and energy production, peaceful use of weapon plutonium, accelerator and spaceship shielding, radiation therapy.
     During the last decade, the measurements of neutron-induced fission cross-sections for some long-lived actinides in the energy range above 20 MeV with continuous spectrum neutrons have been systematically performed only at the WNR/LANSCE facility in Los Alamos and the GNEIS facility in Gatchina. Analysis of the experimental data available in the energy range 20-200 MeV, as well as experience in producing evaluated fission cross-sections below 20 MeV, shows that new independent measurements aimed to improve fission cross-section data base in the energy range above 20 MeV are necessary. At the same time, calculation methods for the fission cross-sections of actinide nuclei at intermediate energies are still under development, except some codes such as ALICE and HETC. In such situation, the semi-empirical formulae based on the few known experimental data are used to estimate the fission cross-sections. These formulae can give not only the systematics for fission cross-section at a certain energy point but also its energy dependence.
     Fission cross-section ratios for 233U, 238U, 232Th, 239Pu and 237Np relative to 235U have been measured using a 50-m flight path. A system of few iron, brass and lead collimators gives the beam diameter of 18 cm at the fission chamber location. The last series of the measurements were carried out with the use of "clearing" magnet placed at 30 m from the source-target. This magnet removes charged particles produced in the collimators and filters from the neutron beam.
     The fission reaction rate was measured using a fast parallel plate ionization chamber with electrode spacing 7 mm and filled with methane working gas. The fission chamber contained 6 foils of oxide fissile material 200 mg/cm2 thick and 18 cm in diameter deposited onto 0.015 cm thick aluminum backings. Also, a weak 252Cf deposit was applied on each fissile foil to match the gains of electronics. The distances between the neutron production target and each fissile foil were determined using 12C neutron transmission resonances. For each isotope under investigation, the time-of-flight and pulse height spectra were accumulated.
     The results of present measurements are shown in Fig. 9,10,11,12,13,14. To obtain fission cross-sections from the measured ratios, the recommended data for fission cross-section of 235U (INDC-368, IAEA, 1997) have been used.The error bars represent the statistical errors only (one standard deviation). The solid lines show JENDL-3.2 data in the energy range below 20 MeV. Also shown are the data of measurements carried out at the WNR/LAMPF facility in Los-Alamos by P.W. Lisowski et al. (1992), P. Staples and K. Morley (1998) and the data of systematics of T. Fukahori (1999) and V.M. Maslov (2000).
     This work was supported by RFBR Grant # 96-02-18012 and ISTC Grant # 609.
Results of GNEIS, Fig.9
Fig. 9. Fission cross-section of 238U in the energy range up to 200 MeV.
Results of GNEIS, Fig.10
Fig. 10. Fission cross-section of 237Np in the energy range up to 200 MeV.
Results of GNEIS, Fig.11
Fig. 11. Fission cross-section of 233U in the energy range up to 200 MeV.
Results of GNEIS, Fig.12
Fig. 12. Fission cross-section of 239Pu in the energy range up to 200 MeV.
Results of GNEIS, Fig.13
Fig. 13. Fission cross-section of 232Th in the energy range up to 200 MeV.
Results of GNEIS, Fig.14
Fig. 14. Low energy part of fission cross-section of 232Th.
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Neutron induced fission cross-sections of lead and bismuth
relative to 235U in the energy range 30 - 200 MeV.

O.A. Shcherbakov, A.B. Laptev, A.S. Vorobyev, A.Y. Donets, A.V. Evdokimov, A.V. Fomichev, Yu.V. Tuboltsev, T. Fukahori
     Among the new applications of the fission data above 20 MeV, the most important are accelerator-driven transmutation of waste reactor materials and energy production, accelerator-based conversion of weapon plutonium and production of tritium, accelerator and spaceship shielding, radiation therapy, etc. During the last years, a need in information about neutron and proton-induced fission of lead and bismuth at intermediate energies increased significantly, mainly due to probable use of these metals as structural materials in the neutron-producing targets of high-current proton accelerators of new generation. Besides, the neutron-induced fission cross-sections of 208Pb and 209Bi are very convenient as standards in the intermediate energy range because they have thresholds at 25-40 MeV, which eliminates the influence of low energy neutrons.
     The fission cross-section ratios for Pb(nat) and 209Bi relative to 235U have been measured using the neutron time-of-flight spectrometer GNEIS. The fission reaction rate was measured using a fast parallel plate ionization chamber. The chamber contained a total of 6 sections, every one containing two pairs of cathode and anode plates spaced by 5 mm. The lead and bismuth targets have been produced from high purity metal using evaporation in vacuum, while for 235U targets the painting technique has been used. The Pb/Bi - fission chamber contained 10 foils of material 260-520 mg/cm2 thick and 1 or 2 foils of 99,992 % enriched 235U 150-260 mg/cm2 thick and 180 mm in diameter, deposited on one side of 0.05-mm-thick aluminum backings. The foils were oriented perpendicular to the neutron beam and all target deposits facing away from neutron source. The distances between the neutron production target and each target foil were determined using carbon (in separate run) and lead (permanently) filters with well-known energies of neutron transmission resonances.
     An absolute normalization of the measured cross-section ratios has been done using the thickness values of the targets and detection efficiencies. Finally, the cross-section ratios have been converted to cross-sections using the recommended reference fission cross-section of 235U of A. Carlson et al. (INDC-368, IAEA, 1997). The results of present measurements are shown in Fig. 15,16 as fission cross-sections of Pb(nat) and 209Bi for the neutron energies from threshold up to 200 MeV together with the experimental data of other authors and parameterizations. The displayed uncertainties of the present data are statistical ones being as much as 4-7 %, 2-3 % and 1.2-1.6 % at 60 MeV, 100 MeV and 200 MeV, respectively.
Results of GNEIS, Fig.15
Fig. 15. Fission cross-section of Pb(nat) in the energy range up to 200 MeV.
Results of GNEIS, Fig.16
Fig. 16. Fission cross-section of 209Bi in the energy range up to 200 MeV.
     The comparison shows that above 45 MeV the present data for Pb(nat) are in a good agreement with the white neutron source measurements with Pb(nat) of P. Staples et al. (1995) at Los Alamos, as well as with the parameterization of A.V. Prokofiev et al. (1998) based on the measurements with Pb(nat) and 208Pb, including the data of P. Staples and other known old and recent experimental data carried out mainly in separate energy points. It can be also seen that the ENDF/HE-VI data based on the on the evaluation of T. Fukahori and S. Perlstein (1991) for 208Pb lies much higher than all experimental data.
     In the case of 209Bi, an agreement of the present data with that of other authors is not so good as for Pb(nat), but also within the stated uncertainties. There is a noticeable discrepancy between our data, as well as the data of P. Staples et al. (1995), and the parameterization of A.N. Smirnov (1997) at neutron energies below ~60 MeV and above ~120 MeV. The ENDF/HE-VI data lies up to 2 times higher than all experimental data below ~150 MeV, but above this energy the tendency to agreement can be seen.
     The data on neutron-induced fission cross-sections of natural Pb and 209Bi presented here were obtained from the measurements carried out jointly by PNPI and KRI in the course of ISTC Project 609-97 in collaboration with the Nuclear Data Center /Japan Atomic Energy Research Institute.
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Multiplicity distributions for fission neutrons emitted from complementary fragments in spontaneous fission of 244Cm, 248Cm and 252Cf.

A.S. Vorobyev, O.A. Shcherbakov, A.B. Laptev, Yu.S. Pleva, V.E. Sokolov, G.A. Petrov, V.A. Kalinin, V.N. Dushin, B.F. Petrov, V.A. Yakovlev, F.-J. Hambsch
     The most direct information about the shape of nascent fission fragments at scission point can be obtained from the number of prompt neutrons emitted from each of the complementary fission fragments. The first neutron multiplicity measurement of this type combined with the direction-sensitive spectroscopy of fission fragments for spontaneous fission of 252Cf has been done at KRI (Russia) [1] more than decade ago, followed by the analogous measurements carried out by the TUD-HMI collaboration (Germany) [2]. These experiments revealed some unusual effects, such as shape-asymmetric cold fission. Recently, a new series of such experiments was started by the PNPI-KRI-IRMM collaboration within the framework of the ISTC Project 554. In the present report the first results of the measurements carried out for spontaneous fission of 244Cm, 248Cm and 252Cf are presented.
     The fission source was placed between two large 200 litre Gd-loaded liquid scintillator tanks which were used for neutron detection in a 2´2p-geometry - to separate contributions from complementary fragments. An efficiency of the neutron registration was about 55% for each detector. A 16-cm thick iron shielding inserted between the tanks was used to decrease both fission neutrons and capture gamma's scattering from one tank into another (cross talks). The fission fragments were collimated toward neutron detectors by means of a pin-hole collimator combined with a common cathode of the twin parallel plate flow-gas ionization chamber with Frish grids. At the counting rate of "useful" events (coincidence of collimated fission fragments) 1-3 s-1, in total about 3·106 of such events for every isotope have been accumulated.
     To deduce mass and kinetic energy distributions of fission fragments, the pulse height data have been corrected for grid inefficiency, pulse height defect, energy losses in the sample, backing and pin-holes. On the basis of reference values of most probable mass and energies of the fission fragments, the provisional distributions have been constructed which then were corrected for mean neutron multiplicities. Neutron multiplicity measurements have been corrected for pile-up effects, background and detector efficiency, including cross talk effects. Detector efficiency have been calculated using Monte-Carlo method and known moments of the prompt neutron multiplicity distribution [3].
     The average neutron multiplicity <n>, total neutron multiplicity nt , variance of n, covariance cov(nl,nh) as a function of total kinetic energy (TKE) and energy distribution are shown in Fig.17(left). The same values except covariance as a function of fragment mass are shown in Fig.17(right). The minimum in n(m), as well as in variance is observed around m=128-129 for all nuclides due to presence of a Z, N magic shells. The average level of variance for 252Cf is twice less then in the data of Signarbieux et al. [4] but in a good agreement with results of Alkhazov et al. [1]. For total neutron multiplicity the increased neutron yield is observed in symmetric fission region for 248Cm and 252Cf unlike to 244Cm.
     The average value of the cov(nl,nh) for 244Cm is approximately twice less then for 248Cm and 252Cf. Variances show rather flat energy dependence except the weak decreasing at lowest and highest values of TKE, that is in a reasonable agreement with results of Alkhazov et al. [1] for 252Cf.
Results of GNEIS, Fig.17
Fig. 17. Energy and mass dependence of average neutron multiplicity <n>, variance s2 and covariance cov(nl,nh) together with energy and mass distribution.
References
1. I.D.Alkhazov, A.V.Kuznetsov, S.S.Kovalenko, B.F.Petrov, V.I.Shpakov. Proc. of Int. Conf. “Nuclear Data for Science and Technology” (30 May–2 June 1988, Mito, Japan). Ed. by S.Igarasi, 1988, p.991-994.
2. I.During, M.Adler, A.Marten, B.Cramer, U.Jahnke. Proc. of Int. Workshop “High-Resolution Spectroscopy of Fission Fragments, Neutrons and Gamma-Rays” (1-2 February 1993, Dresden, Germany). Ed. by H.Marten and K.-D.Schilling, 1993, p.104-113.
3. N.E.Holden, M. S.Zuker. Proc. of Int. Conf. "Nuclear Data for Basic and Applied Science" (13-17 May 1985, Santa Fe, New Mexico, USA). Ed. by P.G.Young, 1985, p.1631-1634.
4. C.Signarbieux, J.Poitou, M.Ribrag, J.Matusze. Phys. Lett. 39B, 503 (1972).
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