EPJ Web of Conferences
Volume 109, 2016The 13th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG2015)
|Number of page(s)||11|
|Section||Underground Nuclear Astrophysics|
|Published online||12 February 2016|
Progress of Jinping Underground laboratory for Nuclear Astrophysics (JUNA)
1 China Institute of Atomic Energy, P. O. Box 275(1), Beijing 102413, China
2 Institute of Modern Physics, Lanzhou, China
3 Tsinghua University, Beijing, China
4 Sichuan University, Chengdu, China
5 Shanghai Jiaotong University, Shanghai, China
6 Monash University, Melbourne, Victoria, Australia
7 RIKEN, Institute of Physical and Chemical Research, Wako, Japan
8 Konkoly Observatory of the Hungarian Academy of Sciences, Hungary
9 South Dakota State University, Brookings, South Dakota, US
10 Minnesota University, Minneapolis and Saint Paul, Minnesota, US
11 University of Notre Dame, Notre Dame, Indiana, US
12 Osaka University, Suita, Osaka, Japan
13 Shandong University, Weihai campus, China
a e-mail: firstname.lastname@example.org
Published online: 12 February 2016
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.
© Owned by the authors, published by EDP Sciences, 2016
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