26.10.2014 Views

JAEA-Data/Code 2007-004 - Welcome to Research Group for ...

JAEA-Data/Code 2007-004 - Welcome to Research Group for ...

JAEA-Data/Code 2007-004 - Welcome to Research Group for ...

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

7.4.3 Solution by Matrix Inversion in Fast Neutron Range<br />

For the fixed source problem in the fast neutron range, the emission rate can be rewritten by<br />

H ig = S ig<br />

+<br />

g<br />

G<br />

∑Σ<br />

smg' →gϕig<br />

' + χ mg ∑νΣ<br />

fmg'<br />

ϕig'<br />

.<br />

g' = 1<br />

g'<br />

= 1<br />

(7.4.3-1)<br />

The fixed source term S ig usually consists of the thermal fission neutron. The scattering term is<br />

determined by the fluxes of the upper energy groups. Given the fast fission term, the fluxes can be<br />

successively solved starting at the highest energy group. The number of the unknowns <strong>to</strong> be<br />

simultaneously solved is the <strong>to</strong>tal number of regions, N.<br />

We have a choice <strong>for</strong> the solution whether by an iterative method or by a matrix inversion. As<br />

far as N is less than about 40, the round-off error due <strong>to</strong> the limited computer precision encountered in<br />

the matrix inversion can be negligible. The computer time required <strong>for</strong> the matrix inversion<br />

(proportional <strong>to</strong> N 3 ) does not so much exceed that <strong>for</strong> the iterative method (proportional <strong>to</strong> the iteration<br />

count*N 2 ). In the SRAC code system, the matrix inversion is applied preferring its definitive solution.<br />

After finding the flux distribution <strong>for</strong> all the energy groups, we have <strong>to</strong> modify the assumed fast<br />

fission source distribution by an iterative process. This power iteration converges rapidly <strong>for</strong> the case<br />

of a thermal reac<strong>to</strong>r because the ratio of fast fission <strong>to</strong> thermal fission is small. Contrary, the procedure<br />

of this section can not be applied <strong>for</strong> the fast reac<strong>to</strong>r where the matrix may have an eigenvalue greater<br />

than unity.<br />

The procedure described in this section is summarized as follows;<br />

Step 1. Normalize the fixed source S ig .<br />

Step 2. Set the initial guess <strong>for</strong> the fast fission distribution.<br />

Step 3. Starting at the highest energy group g=1, calculate emission rates of a group H ig by<br />

Eq.(7.4.3-1).<br />

Calculate fluxes of a group by a matrix inversion.<br />

Repeat Step 3 <strong>for</strong> all groups.<br />

Step 4. Calculate fast fission distributions and modify it by an SOR.<br />

Repeat Step 3 and 4, until the fast fission distribution converges.<br />

7.4.4 Iterative Procedure <strong>for</strong> Eigenvalue Problem in Whole Energy Range<br />

Considering the fact that while the iteration count in the thermal energy range amounts <strong>to</strong><br />

several tens, in the fast energy range any iterative process is not needed, the treatment <strong>for</strong> the thermal<br />

276

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

Saved successfully!

Ooh no, something went wrong!