Progress of Underground Nuclear Astrophysics Experiment JUNA in China

W. P. Liu; Z. H. Li; J. J. He; X. D. Tang; G. Lian; J. Su; Y. P. Shen; Z. An; F. Q. Chao; J. J. Chang; L. H. Chen; H. Chen; X. J. Chen; Y. H. Chen; Z. J. Chen; B. Q. Cui; X. C. Du; X. Fang; C. B. Fu; L. Gan; B. Guo; Z. Y. Han; X. Y. Guo; G. Z. He; J. R. He; A. Heger; S. Q. Hou; H. X. Huang; N. Huang; B. L. Jia; L. Y. Jiang; S. Kubono; J. M. Li; M. C. Li; K. A. Li; E. T. Li; T. Li; Y. J. Li; M. Lugaro; X. B. Luo; H. Y. Ma; S. B. Ma; D. M. Mei; W. K. Nan; W. K. Nan; N. C. Qi; Y. Z. Qian; J. C. Qin; J. Ren; C. S. Shang; L. T. Sun; W. L. Sun; W. P. Tan; I. Tanihata; S. Wang; P. Wang; Y. B. Wang; Q. Wu; S. W. Xu; S. Q. Yan; L. T. Yang; Y. Yang; X. Q. Yu; Q. Yue; S. Zeng; L. Zhang; H. Zhang; H. Y. Zhang; L. Y. Zhang; N. T. Zhang; P. Zhang; Q. W. Zhang; T. Zhang; X. P. Zhang; X. Z. Zhang; W. Zhao; J. F. Zhou; Y. Zhou

doi:10.1007/s00601-022-01735-3

Progress of Underground Nuclear Astrophysics Experiment JUNA in China

W. P. Liu, Z. H. Li, J. J. He, X. D. Tang, G. Lian, J. Su, Y. P. Shen, Z. An, F. Q. Chao, J. J. Chang, L. H. Chen, H. Chen, X. J. Chen, Y. H. Chen, Z. J. Chen, B. Q. Cui, X. C. Du, X. Fang, C. B. Fu, L. GanB. Guo, Z. Y. Han, X. Y. Guo, G. Z. He, J. R. He, A. Heger, S. Q. Hou, H. X. Huang, N. Huang, B. L. Jia, L. Y. Jiang, S. Kubono, J. M. Li, M. C. Li, K. A. Li, E. T. Li, T. Li, Y. J. Li, M. Lugaro, X. B. Luo, H. Y. Ma, S. B. Ma, D. M. Mei, W. K. Nan, W. K. Nan, N. C. Qi, Y. Z. Qian, J. C. Qin, J. Ren, C. S. Shang, L. T. Sun, W. L. Sun, W. P. Tan, I. Tanihata, S. Wang, P. Wang, Y. B. Wang, Q. Wu, S. W. Xu, S. Q. Yan, L. T. Yang, Y. Yang, X. Q. Yu, Q. Yue, S. Zeng, L. Zhang, H. Zhang, H. Y. Zhang, L. Y. Zhang, N. T. Zhang, P. Zhang, Q. W. Zhang, T. Zhang, X. P. Zhang, X. Z. Zhang, W. Zhao, J. F. Zhou, Y. Zhou

School of Physics and Astronomy

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Abstract

Underground Nuclear Astrophysics Experiment in China (JUNA) takes the advantage of the ultra-low background in Jinping underground lab. High current mA level 400 KV accelerator with an ECR source, BGO and neutron detectors were commissioned. JUNA studies directly a number of nuclear reactions important to hydrostatic stellar evolution at their relevant stellar energies. In the first quarter of 2021, JUNA performed the direct measurements of ²⁵Mg (p , γ) ²⁶Al , ¹⁹F (p , α) ¹⁶O , ¹³C (α, n) ¹⁶O and ¹²C(α, γ)¹⁶O near the Gamow window. The experimental results reflect the potential of JUNA with higher statistics, precision and sensitivity of the data. The preliminary results of JUNA experiment and future plan are given.

Original language	English
Article number	43
Number of pages	6
Journal	Few-Body Systems
Volume	63
Issue number	2
DOIs	https://doi.org/10.1007/s00601-022-01735-3
Publication status	Published - Jun 2022

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10.1007/s00601-022-01735-3

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Liu, W. P., Li, Z. H., He, J. J., Tang, X. D., Lian, G., Su, J., Shen, Y. P., An, Z., Chao, F. Q., Chang, J. J., Chen, L. H., Chen, H., Chen, X. J., Chen, Y. H., Chen, Z. J., Cui, B. Q., Du, X. C., Fang, X., Fu, C. B., ... Zhou, Y. (2022). Progress of Underground Nuclear Astrophysics Experiment JUNA in China. Few-Body Systems, 63(2), Article 43. https://doi.org/10.1007/s00601-022-01735-3

@article{d6cae711e1604643a2f1e608c82f46ae,

title = "Progress of Underground Nuclear Astrophysics Experiment JUNA in China",

abstract = "Underground Nuclear Astrophysics Experiment in China (JUNA) takes the advantage of the ultra-low background in Jinping underground lab. High current mA level 400 KV accelerator with an ECR source, BGO and neutron detectors were commissioned. JUNA studies directly a number of nuclear reactions important to hydrostatic stellar evolution at their relevant stellar energies. In the first quarter of 2021, JUNA performed the direct measurements of 25Mg (p , γ) 26Al , 19F (p , α) 16O , 13C (α, n) 16O and 12C(α, γ)16O near the Gamow window. The experimental results reflect the potential of JUNA with higher statistics, precision and sensitivity of the data. The preliminary results of JUNA experiment and future plan are given.",

author = "Liu, {W. P.} and Li, {Z. H.} and He, {J. J.} and Tang, {X. D.} and G. Lian and J. Su and Shen, {Y. P.} and Z. An and Chao, {F. Q.} and Chang, {J. J.} and Chen, {L. H.} and H. Chen and Chen, {X. J.} and Chen, {Y. H.} and Chen, {Z. J.} and Cui, {B. Q.} and Du, {X. C.} and X. Fang and Fu, {C. B.} and L. Gan and B. Guo and Han, {Z. Y.} and Guo, {X. Y.} and He, {G. Z.} and He, {J. R.} and A. Heger and Hou, {S. Q.} and Huang, {H. X.} and N. Huang and Jia, {B. L.} and Jiang, {L. Y.} and S. Kubono and Li, {J. M.} and Li, {M. C.} and Li, {K. A.} and Li, {E. T.} and T. Li and Li, {Y. J.} and M. Lugaro and Luo, {X. B.} and Ma, {H. Y.} and Ma, {S. B.} and Mei, {D. M.} and Nan, {W. K.} and Nan, {W. K.} and Qi, {N. C.} and Qian, {Y. Z.} and Qin, {J. C.} and J. Ren and Shang, {C. S.} and Sun, {L. T.} and Sun, {W. L.} and Tan, {W. P.} and I. Tanihata and S. Wang and P. Wang and Wang, {Y. B.} and Q. Wu and Xu, {S. W.} and Yan, {S. Q.} and Yang, {L. T.} and Y. Yang and Yu, {X. Q.} and Q. Yue and S. Zeng and L. Zhang and H. Zhang and Zhang, {H. Y.} and Zhang, {L. Y.} and Zhang, {N. T.} and P. Zhang and Zhang, {Q. W.} and T. Zhang and Zhang, {X. P.} and Zhang, {X. Z.} and W. Zhao and Zhou, {J. F.} and Y. Zhou",

note = "Funding Information: This work was supported by NSFC under Grant No. 11490560, CNNC innovation fund, CAS instrument fund. Publisher Copyright: {\textcopyright} 2022, The Author(s), under exclusive licence to Springer-Verlag GmbH Austria, part of Springer Nature.",

year = "2022",

month = jun,

doi = "10.1007/s00601-022-01735-3",

language = "English",

volume = "63",

journal = "Few-Body Systems",

issn = "0177-7963",

publisher = "Springer-Verlag London Ltd.",

number = "2",

}

Liu, WP, Li, ZH, He, JJ, Tang, XD, Lian, G, Su, J, Shen, YP, An, Z, Chao, FQ, Chang, JJ, Chen, LH, Chen, H, Chen, XJ, Chen, YH, Chen, ZJ, Cui, BQ, Du, XC, Fang, X, Fu, CB, Gan, L, Guo, B, Han, ZY, Guo, XY, He, GZ, He, JR, Heger, A, Hou, SQ, Huang, HX, Huang, N, Jia, BL, Jiang, LY, Kubono, S, Li, JM, Li, MC, Li, KA, Li, ET, Li, T, Li, YJ, Lugaro, M, Luo, XB, Ma, HY, Ma, SB, Mei, DM, Nan, WK, Nan, WK, Qi, NC, Qian, YZ, Qin, JC, Ren, J, Shang, CS, Sun, LT, Sun, WL, Tan, WP, Tanihata, I, Wang, S, Wang, P, Wang, YB, Wu, Q, Xu, SW, Yan, SQ, Yang, LT, Yang, Y, Yu, XQ, Yue, Q, Zeng, S, Zhang, L, Zhang, H, Zhang, HY, Zhang, LY, Zhang, NT, Zhang, P, Zhang, QW, Zhang, T, Zhang, XP, Zhang, XZ, Zhao, W, Zhou, JF & Zhou, Y 2022, 'Progress of Underground Nuclear Astrophysics Experiment JUNA in China', Few-Body Systems, vol. 63, no. 2, 43. https://doi.org/10.1007/s00601-022-01735-3

TY - JOUR

T1 - Progress of Underground Nuclear Astrophysics Experiment JUNA in China

AU - Liu, W. P.

AU - Li, Z. H.

AU - He, J. J.

AU - Tang, X. D.

AU - Lian, G.

AU - Su, J.

AU - Shen, Y. P.

AU - An, Z.

AU - Chao, F. Q.

AU - Chang, J. J.

AU - Chen, L. H.

AU - Chen, H.

AU - Chen, X. J.

AU - Chen, Y. H.

AU - Chen, Z. J.

AU - Cui, B. Q.

AU - Du, X. C.

AU - Fang, X.

AU - Fu, C. B.

AU - Gan, L.

AU - Guo, B.

AU - Han, Z. Y.

AU - Guo, X. Y.

AU - He, G. Z.

AU - He, J. R.

AU - Heger, A.

AU - Hou, S. Q.

AU - Huang, H. X.

AU - Huang, N.

AU - Jia, B. L.

AU - Jiang, L. Y.

AU - Kubono, S.

AU - Li, J. M.

AU - Li, M. C.

AU - Li, K. A.

AU - Li, E. T.

AU - Li, T.

AU - Li, Y. J.

AU - Lugaro, M.

AU - Luo, X. B.

AU - Ma, H. Y.

AU - Ma, S. B.

AU - Mei, D. M.

AU - Nan, W. K.

AU - Qi, N. C.

AU - Qian, Y. Z.

AU - Qin, J. C.

AU - Ren, J.

AU - Shang, C. S.

AU - Sun, L. T.

AU - Sun, W. L.

AU - Tan, W. P.

AU - Tanihata, I.

AU - Wang, S.

AU - Wang, P.

AU - Wang, Y. B.

AU - Wu, Q.

AU - Xu, S. W.

AU - Yan, S. Q.

AU - Yang, L. T.

AU - Yang, Y.

AU - Yu, X. Q.

AU - Yue, Q.

AU - Zeng, S.

AU - Zhang, L.

AU - Zhang, H.

AU - Zhang, H. Y.

AU - Zhang, L. Y.

AU - Zhang, N. T.

AU - Zhang, P.

AU - Zhang, Q. W.

AU - Zhang, T.

AU - Zhang, X. P.

AU - Zhang, X. Z.

AU - Zhao, W.

AU - Zhou, J. F.

AU - Zhou, Y.

N1 - Funding Information: This work was supported by NSFC under Grant No. 11490560, CNNC innovation fund, CAS instrument fund. Publisher Copyright: © 2022, The Author(s), under exclusive licence to Springer-Verlag GmbH Austria, part of Springer Nature.

PY - 2022/6

Y1 - 2022/6

N2 - Underground Nuclear Astrophysics Experiment in China (JUNA) takes the advantage of the ultra-low background in Jinping underground lab. High current mA level 400 KV accelerator with an ECR source, BGO and neutron detectors were commissioned. JUNA studies directly a number of nuclear reactions important to hydrostatic stellar evolution at their relevant stellar energies. In the first quarter of 2021, JUNA performed the direct measurements of 25Mg (p , γ) 26Al , 19F (p , α) 16O , 13C (α, n) 16O and 12C(α, γ)16O near the Gamow window. The experimental results reflect the potential of JUNA with higher statistics, precision and sensitivity of the data. The preliminary results of JUNA experiment and future plan are given.

AB - Underground Nuclear Astrophysics Experiment in China (JUNA) takes the advantage of the ultra-low background in Jinping underground lab. High current mA level 400 KV accelerator with an ECR source, BGO and neutron detectors were commissioned. JUNA studies directly a number of nuclear reactions important to hydrostatic stellar evolution at their relevant stellar energies. In the first quarter of 2021, JUNA performed the direct measurements of 25Mg (p , γ) 26Al , 19F (p , α) 16O , 13C (α, n) 16O and 12C(α, γ)16O near the Gamow window. The experimental results reflect the potential of JUNA with higher statistics, precision and sensitivity of the data. The preliminary results of JUNA experiment and future plan are given.

UR - http://www.scopus.com/inward/record.url?scp=85128657475&partnerID=8YFLogxK

U2 - 10.1007/s00601-022-01735-3

DO - 10.1007/s00601-022-01735-3

M3 - Article

AN - SCOPUS:85128657475

SN - 0177-7963

VL - 63

JO - Few-Body Systems

JF - Few-Body Systems

IS - 2

M1 - 43

ER -

Progress of Underground Nuclear Astrophysics Experiment JUNA in China

Abstract

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