Abstract
Systematic measurement of the D(p, pp)n cross section at Ep = 13 MeV at star configurations at various inclined angle α is in progress at Kyushu University tandem accelerator laboratory (KUTL). The measured cross section at space star (α = 90°) is about 12% below the recent pd calculation. The next measurement is being made at 0° < α < 90° to see if the large anomaly of about 25% found by the Koln group (2006) at backward α exists also at forward α.
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