JAEA-Conf 2011-002 - 日本原子力研究開発機構
JAEA-Conf 2011-002 - 日本原子力研究開発機構
JAEA-Conf 2011-002 - 日本原子力研究開発機構
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4. Theoretical studies<br />
Theoretical investigations of the surrogate reactions are important since simple<br />
Weisskopf-Ewing approximation is not applicable to low-energy neutron reactions.<br />
Therefore we have to find condition under which the surrogate method really yields<br />
information which can be converted to desired neutron cross sections. Especially, the<br />
capture cross section may deviate by a factor of 5 or more due to the difference of spin<br />
distributions between neutron-induced and surogate reactions[2]. Recently, SC and<br />
Iwamoto have discoved a condition for the surrogate “ratio" method to work[4].<br />
Surrogate ratio method requirs an existence of 2 pairs of neutron-induced and<br />
corresponding surrogate reactions. It was concluded that 1) the weak Weisscopf-Ewing<br />
condition defined in ref. [4] should be satisfied, 2) the 2 surrogate reactions should yield<br />
equivalent spin-parity distributions, and 3) the maximum spin populated by the<br />
surrogate reactions must not be too large (less than 10 hbar) compared to the<br />
neutron-induced reactions. It was demonstrated that even the capture cross section can<br />
be determined with an accuracy of around 10% if they are fulfilled. In ref. [4], however,<br />
the conditions 2) and 3) were simply assumed. Then, we verifed these conditions based<br />
on both quantal[5] and semi-classical[6] models in subsequent works.<br />
The quantal model describes the 238U( 18O, 16O) 240U reaction as a one-step transfer of<br />
a dineutron from 18O to 238U by a three-body piture[5]. The model is formulated as a<br />
Born-approximation with a CDCC (coupled discretized continuum channels) wave<br />
function which includes the breakup effects. The calculated angular distributions<br />
corresponding to different values of spin transfer are shown in Fig. 6. The incident<br />
energy was chosen to be 160 MeV which is close to the energy we are planning in actual<br />
experiments. We notice that this reaction yields a well-defined peak at the grazing<br />
angle, forming a well defined spin distribution. It shows that the whole process proceeds<br />
in the semi-classical manner (like Fresnel diffraction). The transferred spin has a<br />
maximum at 5, and the spin distribution do not depend much on the angle and target<br />
Fig.6 Angular distribution of 16O for<br />
different spin-transfer values (denoted by<br />
numbers) in the 238U( 18O, 16O) 240Ug.s. reaction<br />
at incident energy of 160 MeV[5]<br />
<strong>JAEA</strong>-<strong>Conf</strong> <strong>2011</strong>-<strong>002</strong><br />
<br />
Fig.7 Angular distribution of protons for<br />
different spin-transfer values in the<br />
238U( 3He,p) 240Npg.s.<br />
energy of 30 MeV[5]<br />
reaction at incident