26.02.2013 Views

Program - Brookhaven National Laboratory

Program - Brookhaven National Laboratory

Program - Brookhaven National Laboratory

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

Concerns about the limits of worldwide uranium resources motivated initial interest in the thorium fuel<br />

cycle. It was envisioned that as uranium reserves were depleted, thorium would supplement uranium as a<br />

fuel in nuclear reactors. In thorium fuel cycle, Th-232 is the well known fertile nuclide. It is seen from the<br />

detailed energy dependent neutron-induced cross-section behaviour of this isotope that it supports fission<br />

only with very fast neutrons, i.e. beyond about 1 MeV. At lower energy it has high potential of absorption<br />

of neutrons, and consequently converting to fissile nuclides. In that way, even though Th-232 itself is<br />

not fissile, it transforms into fissile isotope U-233 upon absorption of a neutron. Conversion of fertile to<br />

fissile is possible over a wide energy range, but significant conversion is possible only in an appropriate<br />

range. In a nuclear reactor, the conversion depends on available neutrons over and above what is required<br />

to sustain the fission chain and the inevitable losses due to leakage and parasitic absorption. It must be<br />

noted that the newly generated nuclei undergo all probable interactions and decays, so that they have<br />

both production and destruction routes. It is a challenge to obtain an adequate conversion through a<br />

proper combination of fissile, fertile and other materials arranged in a carefully worked out geometry in<br />

the design. Even before trying with different combination of these factors for achieving better conversion,<br />

one should have a proper and quantified idea about the energy range in which a pure Th-232 isotope<br />

have better conversion in U-233. Since all the parameters such as production and depletion cross sections<br />

involved in the conversion vary with neutron energy due to resonance characteristics which show marked<br />

variation with energy, it becomes very difficult to quantify and select the specific energy range/s in which<br />

the conversion from pure Th-232 sample to U-233 is more favorable. The burnup and depletion codes<br />

such as ORIGEN 2.1 [1] which solve the transmutation and decay equation uses a one group effective<br />

cross section are incapable of generating the behavior of conversion from Th-232 to U-233 with energy. In<br />

the world, none of depletion and radioactive decay computer codes use the point cross section of nuclide<br />

directly. We have developed a computer code which solves the nuclide chain originating with Th-232 with<br />

point cross section. This code is used to estimate the variation of conversion of pure Th-232 sample into<br />

fissile U-233 as a function of neutron energy. In this code, Bateman equations which represent the time<br />

rate of change in the concentration of a specific isotope are solved at every energy point of neutron energy<br />

spectrum. The energy interval is obtained after the proper energy grid unionization process of energy<br />

interval used in each isotope. We have taken point-wise cross section data from the basic evaluated nuclear<br />

data file (ENDF/B-VII.0) for each isotope presented in nuclide chain originating with Th-232. Behaviour<br />

of conversion ratio with energy and with exposure time of pure Th-232 sample is studied in our study with<br />

the help of developed code. The results are also compared using different nuclear data libraries such as<br />

JENDL-3.3.<br />

[1] Allen G Croff, “ORIGEN2: A versatile Computer Code for Calculating the Nuclide Composition and<br />

Characteristic of Nuclear material,” Nuclear technology, 62, 335-352, September 1983.<br />

HE 5 5:00 PM<br />

Remarks on KERMA Factors in ACE files<br />

Chikara Konno, Kentaro Ochiai, Kosuke Takakura, Masayuki Ohta, Satoshi Sato<br />

Japan Atomic Energy Research Institute, Tokai-mura, Naka-gun, Ibaraki-ken 319-1195, Japan<br />

KERMA (Kinematic Energy Release in Material) factors are used as response data in order to obtain<br />

nuclear heating in nuclear analyses. These data are not directly included in nuclear data libraries and<br />

they in ACE (A Compact ENDF) files for the Monte Carlo radiation transport code MCNP are deduced<br />

from cross section data for all the reactions in nuclear data libraries with the NJOY code. Many peoples<br />

often use these data, but little is known concerning fact that most of these data are not always correct.<br />

We will present this issue here. As well known, there are two methods to compute KERMA factors; one<br />

128

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!