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they do not satisfy (for example, because of F2 > 0.50) objective criteria. The successful descriptions of<br />

various GDR decay channels were achieved in the frames of various advanced theoretical models (for example,<br />

[3 - 5]). So the new experimentally-theoretical treatment to the evaluation of partial photoneutron<br />

reaction cross sections was proposed [6]. That uses both the results of modern preequilibrium calculations<br />

based on the Fermi-gas densities equations and taking into account the effects of nuclear deformation and<br />

GDR isospin splitting [4, 5] and experimental data for only (γ,xn) reaction cross section, free from outgoing<br />

neutrons multiplicity sorting uncertainties and errors. Theoretically calculated transitional multiplicity<br />

functions Fi theor were used for partial reaction cross section σ eval (γ,in) evaluation of by the way - σ eval (γ,in)<br />

= Fi theor (γ,in) x σ exp (γ,xn). New reliable and authentic data on partial and total photoneutron reaction<br />

((γ,sn) = (γ,n) + (γ,2n) + (γ,3n) + ...) cross sections were evaluated for nuclei mentioned above. It<br />

was shown that those are in contradiction to data obtained using the neutron multiplicity sorting method<br />

but are in agreement with data obtained using the method of induced activity - direct method of partial<br />

reaction cross section determination free of neutron multiplicity problems. Various physical consequences<br />

of ”evaluated-experimental” distinctions of data are discussed. The work was supported by Russia Grant<br />

of Scientific Schools Supporting 02.120.21.485-SS, MINOBRNAUKA Contract 02.740.11.0242 and RFBR<br />

Grant N 09-02-00368.<br />

Corresponding author: V.V.Varlamov<br />

[1] E.Wolynec et al., Revista Brasileira Fisica, 17 56 (1987). [2] V.V.Varlamov et al., INDC(CCP)-<br />

440, IAEA NDS, Vienna, Austria, 37 (2004). [3] M.B.Chadwick et al., Phys.Rev. C44 814 (1991).<br />

[4] B.S.Ishkhanov et al., Physics of Particles and Nuclei, 38 bf232 (2007). [5] B.S.Ishkhanov et al., Physics<br />

of Atomic Nuclei, 71 493 (2008). [6] V.V.Varlamov et al., Bull. Rus. Acad. Sci. Phys. 74 842 (2010).<br />

PR 88<br />

The Systematics of (n,2n) Reaction Excitation Function<br />

Jimin Wang, Xi Tao, Xiaolong Huang, Youxiang Zhuang, China Nuclear Data Center, China Institute of<br />

Atomic Energy, CHINA.<br />

Based on the constant temperature evaporation model taking the competition of (n,3n) reaction and the<br />

contribution of preequilibrium emission into account, the systematics formulae of (n,2n) reaction excitation<br />

function have been established. The systematics behaviours of (n,2n) reaction excitation function have been<br />

studied. There are two systematics parameters T and σn,M, and can be adjusted in the formulae. For<br />

getting the two parameters, the new evaluated data of (n,2n) reactions were adopted and fitted by means<br />

of the nonlinear least squares method. The fitted results agree fairly well with the measured data at<br />

45 < A < 210 below 30 MeV. Based on a body of new measurements, the reliability to predict (n,2n)<br />

reaction excitation function is improved. Hence more accurate systematics prediction for unmeasured<br />

nucleus or energy range may be provided.<br />

PR 89<br />

Analysis of Deuteron Induced Reactions from Threshold<br />

Tao Ye, Weili Sun, Jia Wang, Institute of Applied Physics and Computational Mathematics, Beijing<br />

100094, China. Yukinobu Watanabe, Department of Advanced Energy Engineering Science, Kyushu<br />

University, Kasuga, Fukuoka 816-8580, Japan. Kazuyuki Ogata, Research Center of Nuclear Physics<br />

(RCNP), Osaka University, Ibaraki 567-0047, Japan.<br />

308

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