We review the current scenario of long-duration Gamma-ray burst (LGRB) progenitors, and in addition, present models massive stars for a mass range $10\text{--}150 \, \mathrm{M}_\odot$ with $\Delta \mathrm{M}=10 rotation rate $v/v_{\rm{crit}}=0$ to $0.6$ velocity resolution v/v_{\rm{crit}} =0.1$. further discuss possible metallicity distribution from our that might be preferable creation success...