Zobrazeno 1 - 10
of 25
pro vyhledávání: '"Ma, NanRu"'
Publikováno v:
In Science Bulletin 30 April 2023 68(8):775-778
Publikováno v:
He jishu, Vol 46, Iss 8, Pp 080006-080006 (2023)
Through the use of the accelerator facilities at home and abroad, the nuclear reaction group of the China Institute of Atomic Energy has made many remarkable achievements in the study of fusion-fission dynamics, fusion-enhancement mechanisms at sub-b
Externí odkaz:
https://doaj.org/article/2e4fa11957324d5c9ea4cd0279e5e089
Autor:
Bao, Pengfei, Lin, Chengjian, Yang, Feng, Guo, Zhaoqiao, Guo, Tianshu, Yang, Lei, Sun, Lijie, Jia, Huiming, Xu, Xinxing, Ma, Nanru, Zhang, Huanqiao, Liu, Zuhua
The quadrant silicon detector, a kind of passivated implanted planar silicon detector with quadrant structure on the junction side, gained its wide application in charged particle detection. In this paper, the manufacturing procedure, performance tes
Externí odkaz:
http://arxiv.org/abs/1401.7324
Direct measurement of the 26Si(α, p)29P reaction at CRIB for the nucleosynthesis in the X-ray bursts
Autor:
Okawa Kodai, Kim Minju, Chae Kyungyuk, Hayakawa Seiya, Adachi Satoshi, Cha Soomi, Chillery Thomas William, Furuno Tatsuya, Gu Gyungmo, Hanai Shutaro, Imai Nobuaki, Kahl David, Kawabata Takahiro, Kim Chanhee, Kim Dahee, Kim Sohyun, Kubono Shigeru, Kwag Minsik, Li Jiatai, Ma Nanru, Michimasa Shin’ichiro, Nguyen Kim Uyen, Nguyen Ngoc Duy, Sakanashi Kohsuke, Shimizu Hideki, Sirbu Oana, Yamaguchi Hidetoshi, Yokoyama Rin, Zhang Qian
Publikováno v:
EPJ Web of Conferences, Vol 275, p 02009 (2023)
Several (α, p) reactions with radioactive-ions (RI) in the αp-process are important to characterize X-ray bursts. However, some of them do not have sufficient experimental data, and the 26Si(α, p)29P reaction is one of such reactions. We performed
Externí odkaz:
https://doaj.org/article/121aeffef29b4663a72fa678ceb3210d
Autor:
Liu, Qiang, Ye, Yanlin, Li, Zhihuan, Lin, Chengjian, Jia, Huiming, Ge, Yucheng, Li, Qite, Lou, Jianling, Yang, Xiaofei, Yang, Biao, Feng, Jun, Zang, Hongliang, Chen, Zhiqiang, Liu, Yang, Liu, Wei, Chen, Sidong, Yu, Hanzhou, Li, Jingjing, Zhang, Yun, Yang, Feng, Yang, Lei, Ma, Nanru, Sun, Lijie, Wang, Dongxi
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 21 July 2018 897:100-105
Autor:
A. A. Oliva, A. Tumino, N. Soic, P. M. Prajapati, L. Acosta, R. Alba, F. Barba, S. Cherubini, G. D’Agata, D. Dell’Aquila, A. Di Pietro, J.P. Fernandez, P. Figuera, D. Galaviz Redondo, L. Guardo, M. Gulino, F. Hammache, D. Jelavic Malenica, A.I. Kiliç, M. La Cognata, M. La Commara, L. Lamia, D. Lattuada, C. Maiolino, G. Manicò, M. Mazzocco, M. Milin, Ma Nanru, A. Nurmukhanbetova, D. Nurkic, S. Palmerini, T. Parascandolo, D. Pierroutsakou, R.G. Pizzone, R. Popocovski, G.G. Rapisarda, S. Romano, D. Santonocito, M.L. Sergi, A. Shotter, R. Spartà, A. Spiridon, L. Trache, N. Vukman, H. Yamaguchi
12C +12 C is the main reaction during core and shell carbon burning in massive stars, however, at temperatures higher than 109K when most of the carbon is depleted and its abundance is lower than 16O, the 12C +16 O fusion can also become relevant. Mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d6ccaa6cadc3b0aabcc2a45eff433f6
https://hdl.handle.net/20.500.11769/558663
https://hdl.handle.net/20.500.11769/558663
Autor:
A.A. Oliva, A. Tumino, N. Soic, M.P. Prajapati, L. Acosta, R. Alba, F. Barba, S. Cherubini, G. D’Agata, D. Dell’Aquila, A. Di Pietro, P.J. Fernandez, P. Figuera, D. Galaviz Redondo, L. Guardo, M. Gulino, F. Hammache, D. Jelavic Malenica, A.I. Kiliç, M. La Cognata, M. La Commara, L. Lamia, D. Lattuada, C. Maiolino, G. Manicò, M. Mazzocco, M. Milin, Ma Nanru, A. Nurmukhanbetova, D. Nurkic, S. Palmerini, T. Parascandolo, D. Pierroutsakou, R.G. Pizzone, R. Popocovski, G.G. Rapisarda, S. Romano, D. Santonocito, M.L. Sergi, A. Shotter, R. Spartà, A. Spiridon, L. Trache, N. Vukman, H. Yamaguchi
The carbon-burning process in massive stars mainly occurs via the 12C +12 C. However, at temperatures higher than 109K and considering the increased abundance of 16O produced during the later stages of the heliumburning,the 12C+16O fusion can also be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::30ec1accd2af6e1d0672088ddc277306
https://hdl.handle.net/20.500.11769/558666
https://hdl.handle.net/20.500.11769/558666
Autor:
Ma Nanru, Lin Chengjian, Jia Huiming, Xu Xinxing, Yang Feng, Yang Lei, Sun Lijie, Wang Dongxi, Zhang Huanqiao, Liu Zuhua
Publikováno v:
EPJ Web of Conferences, Vol 239, p 01007 (2020)
Surrogate reaction method is an important approach to overcome the difficulties meet in the direct measurement of neutron induced nuclear reaction. The current existing surrogate reactions generally employ the peripheral reactions such as inelastic e
Externí odkaz:
https://doaj.org/article/59a8af3675964267bb69fabec48cab94
Autor:
Yang Lei, Lin Chengjian, Jia Huiming, Ma Nanru, Wang Dongxi, Yang Feng, Sun Lijie, Xu Xinxing, Wen Peiwei, Zhong Fupeng
Publikováno v:
EPJ Web of Conferences, Vol 223, p 01071 (2019)
We will introduce some new results derived recently by the nuclear reaction group at China Institute of Atomic Energy, on the properties of the optical model potentials of neutron-halo 6He system and reaction mechanisms induced by proton-drip line nu
Externí odkaz:
https://doaj.org/article/2953529c0c404ef18c596121203caf70
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