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Report No.
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Nuclear astrophysics at TRIAC facility

Miyatake, Hiroari

The neutrino driven wind model at core collapse supernovae is one of proposed scenarios explaining the origin of the element synthesis through the rapid neutron capture. My talk report the systematic direct measurements of the $$^8$$Li($$alpha$$,n)$$^{11}$$B reaction and so on, in order to clear the seed to neutron ratio, which is an important parameter to explain the heavy elemental abundance pattern. Based on the measurements, I indicate the dominant reaction flow as a function of the temperature at the stage of the alpha process, which is a prior process to the rapid neutron capture.

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