For explosive hydrogen burning environments such as classical novae and typeⅠX-ray bursts,our current understanding of nucleosynthesis and energy generation in these astrophysical scenarios is limited by the uncertainties in particular thermonuclear reaction rates.The For explosive hydrogen burning environments such as classical novae and type I-ray bursts, our current understanding of nucleosynthesis and energy generation in these astrophysical scenarios is limited by the uncertainties in particular thermonuclear reaction rates.