Jinping Underground lab for Nuclear Astrophysics (JUNA) will take the advantage of the ultralow background in Jinping underground lab, high current accelerator based on an ECR source and highly sensitive detector to study directly a number of crucial reactions to the hydrostatic stellar evolution for the first time at their relevant stellar energies. In its first phase, JUNA aims at the direct measurements of 25Mg(p,γ)26Al, 19F(p,α)16O, 13C(α,n)16O and 12C(α,γ)16O. The experimental setup, which include the accelerator system with high stability and high intensity, the detector system, and the shielding material with low background, will be established during the above research. The current progress of JUNA will be given.
|Original language||English (US)|
|Journal||EPJ Web of Conferences|
|State||Published - Feb 12 2016|
|Event||13th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2015 - Beijing, China|
Duration: Jun 24 2015 → Jun 27 2015
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