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

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i.e.,<br />

X 0 j / X j = 1 ( j ∉ R)<br />

. (7.3.3-11)<br />

Under these assumptions, Eq.(7.3.3-8) can be rewritten as<br />

⎛<br />

⎞<br />

ϕ ⎜<br />

⎟<br />

i<br />

( u)<br />

→ X −<br />

→ ∞<br />

0i<br />

∑γ<br />

ij<br />

X<br />

i<br />

<strong>for</strong> X<br />

i . (7.3.3-12)<br />

⎝ j∉R<br />

⎠<br />

On the other hand, an equivalent theorem between homogeneous and heterogeneous systems<br />

means that the flux in the absorber lump should be expressed by the spectrum in homogeneous<br />

medium<br />

X 0i<br />

+ bi<br />

ϕ i ( u)<br />

= → ( X 0i<br />

+ bi<br />

) / X i <strong>for</strong> X i → ∞ . (7.3.3-13)<br />

X + b<br />

i<br />

i<br />

where the flux is normalized <strong>to</strong> be unity at off-resonance energy.<br />

For Eqs.(7.3.3-12) and (7.3.3-13) <strong>to</strong> be held, the following identity must be satisfied:<br />

bi<br />

= −<br />

∑<br />

j∉R<br />

γ<br />

ij<br />

(7.3.3-14)<br />

For a special case where the unit cell under study consists of fuel region (f) and modera<strong>to</strong>r region (m),<br />

we can prove the conventional relation 61)<br />

b<br />

i<br />

= − γ = 1 − C , (7.3.3-15)<br />

fm<br />

where C is the Dancoff correction fac<strong>to</strong>r and<br />

− γ fm corresponds <strong>to</strong> the first-flight blackness <strong>for</strong><br />

neutrons leaving the fuel region 61) . Figure 7.3.3-1 shows the expression of b i <strong>for</strong> other simple<br />

geometries.<br />

Consequently, from the above examples, Eq.(7.3.3-14) is considered <strong>to</strong> be a generalization of<br />

the previous works introduced in the previous section. Equation (7.3.3-14) shows that the Dancoff<br />

correction fac<strong>to</strong>r <strong>for</strong> complex geometry can be obtained by calculating the generalized blackness γ fm .<br />

Here, the blackness γ fm is calculated by using the collision probability package in the SRAC system,<br />

that is, by using the value of P ij <strong>for</strong> a sufficiently large value of Σ ( j ∈ R)<br />

, as Σ j =300 cm -1 , based on<br />

Eq.(7.3.3-5).<br />

j<br />

256

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