03.04.2013 Views

Fission Product Yield Data for the Transmutation of Minor Actinide ...

Fission Product Yield Data for the Transmutation of Minor Actinide ...

Fission Product Yield Data for the Transmutation of Minor Actinide ...

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.

hand, <strong>the</strong> on average longer half-lives <strong>of</strong> <strong>the</strong> less<br />

neutron rich fission products also give rise to an<br />

advantage. Part <strong>of</strong> <strong>the</strong> primary fission products,<br />

which remain after post-scission neutron<br />

evaporation by <strong>the</strong> fragments, occur with longer<br />

half-lives and hence are easier to observe. They can<br />

now be measured directly, instead <strong>of</strong> only through<br />

<strong>the</strong>ir beta decay products.<br />

4.6.3.2. Sub-actinide fission<br />

4.6.3.2.1. Mass distributions<br />

For each sub-actinide target, <strong>the</strong> mass distribution<br />

is extracted from <strong>the</strong> measured cumulative<br />

and independent isotope yields by fitting simultaneously<br />

<strong>the</strong> mass and charge distribution. The fission<br />

process is assumed to be symmetric <strong>for</strong> <strong>the</strong> subactinide<br />

targets. There<strong>for</strong>e, <strong>the</strong> mass and <strong>the</strong> charge<br />

distribution <strong>for</strong> a given mass are each described by a<br />

single Gaussian in <strong>the</strong> fit. Moreover, <strong>the</strong> assumption<br />

is made that <strong>the</strong> most probable charge, as well as <strong>the</strong><br />

width <strong>of</strong> <strong>the</strong> charge distribution, vary linearly with<br />

<strong>the</strong> mass <strong>of</strong> <strong>the</strong> fission fragment. The following<br />

parameterization <strong>of</strong> <strong>the</strong> production cross-section as<br />

a function <strong>of</strong> <strong>the</strong> mass and charge <strong>of</strong> <strong>the</strong> fission<br />

fragment is adopted:<br />

-<br />

2 1<br />

s prod ( AZ , ) = lAe<br />

A Âe<br />

p G<br />

212<br />

2 ( A-M ) ( Z-- i Z )<br />

A<br />

p<br />

2<br />

G G<br />

(4.6.1)<br />

with Z p = m 1 + m 2 A and G Z = g 1 + g 2 A. The first<br />

Gaussian represents <strong>the</strong> symmetric mass distribution<br />

defined by <strong>the</strong> height l A , mean M A and<br />

width G A . The rest <strong>of</strong> <strong>the</strong> <strong>for</strong>mula reflects <strong>the</strong> charge<br />

distribution. In <strong>the</strong> case <strong>of</strong> an independent yield,<br />

only one term in <strong>the</strong> sum <strong>of</strong> <strong>the</strong> normalized<br />

Gaussian charge distribution (i.e., i = 0) contributes.<br />

A cumulative yield is described by summing <strong>the</strong><br />

contributions <strong>of</strong> neighbouring isobars. The index i is<br />

equal to 0, 1,…5 <strong>for</strong> neutron rich cumulative yields,<br />

and equal to 0, –1,…–5 <strong>for</strong> neutron deficient<br />

cumulative yields. The number <strong>of</strong> terms (six) in <strong>the</strong><br />

summation <strong>for</strong> cumulative yields is ra<strong>the</strong>r arbitrary,<br />

but in <strong>the</strong>se investigations has turned out to be<br />

sufficient. A more elaborate description <strong>of</strong> <strong>the</strong><br />

functional <strong>for</strong>m can be found in <strong>the</strong> work by<br />

Hagebø and Lund [4.6.24].<br />

The values <strong>of</strong> <strong>the</strong> fit parameters obtained <strong>for</strong><br />

all sub-actinide targets are tabulated in Table 4.6.2.<br />

Z<br />

i<br />

Z<br />

2<br />

The mean value as well as <strong>the</strong> height <strong>of</strong> <strong>the</strong> mass<br />

distribution clearly increases with increasing target<br />

mass, as expected. From <strong>the</strong> mean <strong>of</strong> <strong>the</strong> mass distributions<br />

it can be concluded that, on average, nine<br />

mass units are emitted be<strong>for</strong>e and after fission. With<br />

<strong>the</strong> charge distribution known from <strong>the</strong> fit <strong>of</strong><br />

Eq. (4.6.1), it is straight<strong>for</strong>ward to determine <strong>the</strong><br />

fractional independent or cumulative yields<br />

represented by each <strong>of</strong> <strong>the</strong> observed independent or<br />

cumulative isotope yields in <strong>the</strong>ir mass chains.<br />

Subsequently, <strong>the</strong> measured yields are divided by<br />

<strong>the</strong>ir corresponding fractional yields to derive <strong>the</strong><br />

experimental mass yields. In <strong>the</strong> case <strong>of</strong> nat Pb, <strong>the</strong><br />

spread in <strong>the</strong> adjusted yields is ra<strong>the</strong>r large.<br />

There<strong>for</strong>e, <strong>the</strong> final mass distribution has been<br />

obtained after fitting to <strong>the</strong> measured yields, which<br />

represent at least 50% <strong>of</strong> <strong>the</strong> complete mass distribution.<br />

The total mass yields are plotted in<br />

Fig. 4.6.1, toge<strong>the</strong>r with <strong>the</strong> mass distribution<br />

obtained in <strong>the</strong> fit <strong>for</strong> nat W, 197 Au, nat Pb and 208 Pb.<br />

The results agree with <strong>the</strong> assumption <strong>of</strong> a<br />

symmetric mass and charge distribution.<br />

4.6.3.2.2. Charge distributions<br />

Integrating over <strong>the</strong> Gaussian and multiplying<br />

by a factor 1/2, because <strong>of</strong> <strong>the</strong> two fission fragments<br />

in each fission event, gives an estimate <strong>for</strong> <strong>the</strong><br />

fission cross-section. The values <strong>for</strong> <strong>the</strong> fission<br />

cross-sections determined in this way are also given<br />

in Table 4.6.2. The assumption is made that <strong>the</strong><br />

uncertainties in <strong>the</strong> independent and cumulative<br />

yields that have been used in <strong>the</strong> fit are uncorrelated,<br />

since <strong>the</strong>y stem from many different spectra.<br />

There<strong>for</strong>e <strong>the</strong> only uncertainty remaining in <strong>the</strong><br />

deduced fission cross-sections is <strong>the</strong> systematic<br />

uncertainty due to <strong>the</strong> overall normalization<br />

determined from <strong>the</strong> proton flux. Eismont et al.<br />

[4.6.25] have made a data compilation <strong>for</strong> <strong>the</strong> fission<br />

cross-section as a function <strong>of</strong> incident proton energy<br />

<strong>for</strong> some <strong>of</strong> <strong>the</strong>se target materials. The values from<br />

<strong>the</strong> Eismont et al. fit are also shown in Table 4.6.2<br />

<strong>for</strong> comparison and are in fairly good agreement<br />

with <strong>the</strong> results from this work.<br />

By fitting Eq. (4.6.1) to <strong>the</strong> available experimental<br />

independent and cumulative yields,<br />

in<strong>for</strong>mation on <strong>the</strong> charge distribution is obtained.<br />

The charge distributions in three fission fragment<br />

mass regions <strong>of</strong> 208 Pb are shown in Fig. 4.6.2 as an<br />

example. The fitted charge distributions are<br />

evaluated <strong>for</strong> <strong>the</strong> indicated masses. Since <strong>the</strong> charge<br />

yield curves vary only slowly as a function <strong>of</strong> mass,<br />

<strong>the</strong> fits should give a good representation <strong>of</strong> <strong>the</strong>

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

Saved successfully!

Ooh no, something went wrong!