Speaker
Description
The characteristic 1.157 MeV $\gamma$-rays from the radioactive decay of $^{44}$Ti ($t_{1/2}$ = 59.1 y) provide information about supernova explosion phenomena. The study of $^{44}$Ti($\alpha$,$p$)$^{47}$V reaction rates is essential for predicting the abundance of $^{44}$Ti. To study the properties of energy levels in $^{48}$Cr, $^{50}$Cr($p$,$t$)$^{48}$Cr reaction will be performed at the JAEA-Tokai tandem accelerator facility. The $^{50}$Cr($p$,$t$)$^{48}$Cr reaction will be measured using the proton beam and $^{50}$Cr target in normal kinematics. The recoiling particles will be detected using silicon detector telescopes. The astrophysical interest energy region of $E_{x}$ = 8 – 10 MeV will be studied. Details of the experiment will be discussed.
