JINA - Virtual Journal of Nuclear Astrophysics,
17 December 2021
Volume 19, Issue 51 (21 Articles)
- # 2 - First application of mass measurement with the Rare-RI Ring reveals the solar r-process abundance trend at A=122 and A=123. (arXiv:2112.05312v1 [nucl-ex])
- H. F. Li, S. Naimi, T. M. Sprouse, M. R. Mumpower, Y. Abe, Y. Yamaguchi, D. Nagae, F. Suzaki, M. Wakasugi, H. Arakawa, W.B. Dou, D. Hamakawa, S. Hosoi, Y. Inada, D.Kajiki, T. Kobayashi, M. Sakaue, Y. Yokoda, T. Yamaguchi, R. Kagesawa, D. Kamioka, T.Moriguchi, M. Mukai, A. Ozawa, S. Ota, N. Kitamura, S. Masuoka, S. Michimasa, H. Baba, N. Fukuda, Y. Shimizu, H. Suzuki, H. Takeda, D.S. Ahn, M. Wang, C.Y. Fu, Q. Wang, S.Suzuki, Z. Ge, Yu. A. Litvinov, G. Lorusso, P. M. Walker, Zs. Podolyak, T. Uesaka
- http://arxiv.org/abs/2112.05312
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.
