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Program - Brookhaven National Laboratory

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The optical model has a significant impact on many branches of nuclear reaction physics. The central<br />

assumption of that model is that the complicated interaction between an incident particle and a nucleus can<br />

be represented by a complex mean-field potential. An important feature of a good optical model potential is<br />

that it can be used to reliably predict these observables for energies and nuclides for which no experimental<br />

measurement data exist, while the ingredients of the model, either microscopic or phenomenological, are<br />

physically well-behaved. From the view of the many-body theory the nucleon optical potential can be<br />

identified with the mass operator of the one-particle Green function. The first and second order mass<br />

operators of one particle Green function in nuclear matter are obtained, and the real and imaginary parts<br />

of the optical potential for finite nuclei are obtained by applying a local density approximation. With certain<br />

versions of the Skyrme interactions we have obtained the microscopic optical potential for finite nuclei which<br />

shows that for certain energy regions the potential depth, shape, relative contributions of the surface and<br />

volume parts, as well as the energy dependences are in reasonable agreement with the phenomenological<br />

optical potentials and those based on realistic nucleon-nucleon interaction. The calculated results, such as<br />

the total, nonelastic and differential cross sections and analyzing powers are in good agreement with the<br />

experimental data and to certain extent comparable with the phenomenological optical potentials up to<br />

100 MeV. The microscopic optical potentials for deuteron, helium-3 and alpha are obtained by the twoparticle,<br />

the three-particle and four-particle Green function method through nuclear matter approximation<br />

and local density approximation based on the effective Skyrme interaction. The radial dependence, the<br />

volume integral per nucleon and the root mean square (rms) radii of the microscopic optical potential<br />

are calculated. The reaction cross sections and elastic scattering angular distributions for nuclides in the<br />

mass range 12≤ A ≤ 208 with incident deuteron, helium-3 and alpha energies from threshold up to 100<br />

MeV per nucleon are calculated, and the calculated results are compared with the experimental data. The<br />

calculated results of reaction cross sections and elastic scattering angular distributions are generally in<br />

good agreement with the experimental data in most cases.<br />

PR 103<br />

Experimental Average Prompt Neutron Multiplicity as a Function of Total Kinetic Energy<br />

of Fission Fragments Described by Point-by-Point Model Calculations<br />

Iuliana Visan, Institute for Nuclear Research, POB 78, 115400-Mioveni, AG, Romania. Anabella Tudora,<br />

University of Bucharest, Faculty of Physics, Bucharest-Magurele, POB MG-11, R-76900, Romania.<br />

The Point by Point (PbP) model calculations of the average prompt neutron multiplicity as a function<br />

of total kinetic energy (TKE) describe very well the experimental data of 252Cf (SF), 239Pu (nth,f)<br />

and 235U(nth,f) over the entire TKE range, including not only the slope (dTKE/dν)-1 but also the flat<br />

or decreasing behaviour at low TKE values. Present deterministic PbP model results of (TKE) are<br />

analyzed comparatively with previous PbP (TKE) results based on the same multi-parametric matrix<br />

ν (Z, A, TKE) and different manners of averaging this matrix over the fission fragment distributions, as well<br />

as with previous and recent results of probabilistic Monte-Carlo treatments. The PbP treatment provides<br />

average model parameters as a function of TKE that are used in the most probable fragmentation approach<br />

giving (TKE) in very good agreement with experimental data, too. The most probable fragmentation<br />

with average parameters depending on TKE has the advantage to predict (TKE) outside the TKE<br />

range where experimental FF distributions exist and offers the possibility to provide results at many<br />

TKE values in a very short calculation time compared to PbP and Monte-Carlo treatments. Possible<br />

explanations of discrepancies between the slopes of different sets of experimental (TKE) data are<br />

mentioned, too. Experimental fission fragment distributions Y (A, TKE) recently measured for 234U (n,<br />

f) at more incident neutron energies covering the range from 0 2 MeV up to 5 MeV allow the PbP model<br />

prediction of (TKE) for this fissioning system.<br />

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