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TRIAC Progress Report - KEK

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GEM-MSTPC among the accumulated data. Figure 3-9 shows a typical example of true<br />

reaction. The data analysis for selecting true reaction events on event-by-event bases is<br />

in progress.<br />

Fig. 3-9. Typical event pattern of 8 Li(α, n) 11 B reaction. (Left): Energy losses measured by pad<br />

(dE/pad) are presented as a function of the number of anode pads, where the beam comes in from the<br />

low pad number. (Right): Horizontal (x) and vertical (y) positions of the three-dimensional particle<br />

trajectories, where the beam direction was defined as the z-axis (i.e. increasing pad numbers in the<br />

figures).<br />

Using a stable ion beam of 4 He provided by the <strong>TRIAC</strong>, the RNB-KJ04<br />

(Spokesperson: H. Makii (JAEA) and H. Miyatake (JAEA), Collaboration: <strong>KEK</strong> (9),<br />

JAEA (5), RIKEN (1), Osaka Univ. (1)) was proposed to directly measure the 12 C(α,<br />

γ) 16 O reaction cross sections and determine the strength of electric-dipole (E1) and/or<br />

-quadrupole (E2) components in the α-capture cross sections (decaying strength of<br />

excited 16 O by emitting γ-rays of corresponding multi-polarities) at stellar energies. The<br />

reaction plays an important role at the stage of helium-burning in stellar evolution; its<br />

reaction rate determines the mass fraction of 12 C and 16 O after the stellar helium-burning,<br />

the abundance of elements from oxygen to iron, and the iron-core mass before<br />

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