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The  19 F( p ,  αγ ) 16 O reaction is of crucial importance for Galactic  19 F abundances and CNO cycle loss in first generation Population III stars. Due to its extremely small cross sections, the  19 F( p ,  αγ ) 16 O reaction has not been measured in the low energy part of the Gamow window(70-200 keV). As a day-one campaign, the experiment was performed under the extremely low cosmicray-induced background environment of the China JinPing Underground Laboratory(CJPL), one of the deepest underground laboratories in the world. The  γ -ray yields were measured over E  c   .   m   .  =72.4–344 keV, covering the full Gamow window for the first time. The direct experimental data will help people to expound the fluorine over-abundances, energy generation, as well as heavy-element nuclosynthesis scenario in asymptotic giant branch (AGB) stars, with the astrophysical model on the firm ground.

Direct measurement of the 19F(p, αγ)16O reaction in JUNA

Direct measurement of the ¹⁹F(p, αγ)¹⁶O reaction in JUNA