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| 1 | FOREWORD显示文摘In the past year of 2013,CIAE had actively conducted science and technology innovation campaigns,with innovation capability and the resulting benefits improving steadily.213 projects had been in progress,and 54 projects were newly initiated.24 projects had passed related verifications,and 30 projects had won awards of different levels,including National Prize for Progress in Science and Technology。 | Wan gang | 2013 | Annual Report of China Institute of Atomic Energy2013，，1： | 1 |
| 2 | Research Progress of Nuclear Astrophysics Physics:Progress of Jinping Underground Laboratory for Nuclear Astrophysics Experiment JUNA显示文摘1 Progress of this program This program is supported by the China Jinping Underground Laboratory(CJPL)and the direct measurement of stellar key reactions of(α,γ),(α,n),(p,γ)and(p,α)will be precisely carried out at the merit of current project by utilizing high stability and intensity accelerator,high efficiency detector and the shielding of extremely low background. | LIU Wei-ping LI Zhi-hong HE Jian-jun TANG Xiao-dong LIAN Gang GUO Bing AN Zhu CHEN Qing-hao CHEN Xiong-jun CHEN Yang-ping CHEN Zhi-jun CUI Bao-qun DU Xian-chao FU Chang-bo GAN Lin HAN Zhi-yu HE Guo-zhu A.Heger HOU Su-qing HUANG Han-xiong HUANG Ning JIA Bao-lu JIANG Li-yang S.Kubono LI Jian-min LI Kuo-ang LI Tao LI Xin-yue LI Yun-ju M.Lugaro LUO Xiao-bing MA Shao-bo MEI Dong-ming QIAN Yong-zhong QIN Jiu-chang REN Jie SU Jun SUN Liang-ting TAN Wan-peng I.Tanihata WANG Peng WANG You-bao WU Qi XU Shi-wei YAN Sheng-quan YANG Li-tao YU Xiang-qing YUE Qian ZENG Sheng ZHANG Huan-yu ZHANG Hui ZHANG Li-yong ZHANG Ning-tao ZHANG Qi-wei ZHANG Tao ZHANG Xiao-peng ZHANG Xue-zhen ZHANG Zi-min ZHAO Wei ZHAO Zhuo ZHOU Chao ZHOU Yong | 2015 | Annual Report of China Institute of Atomic Energy2015，，1： | 0 |
| 3 | Stellar reaction rate of 55Ni(p,γ)56Cu in Type I X-ray bursts显示文摘^56Cu is close to the waiting-point nucleus ^56Ni and lies on the rapid proton capture (rp) process path in Type I X-ray bursts (XRBs). In this work, we obtained a revised thermonuclear reaction rate of ^55Niep;cT56Cu in the temperature region relevant to XRBs. This rate was recalculated based on the recent experimental level structure in ^56Cu, the recently measured proton separation energy of Sp = 579.8(7.1) keV, together with shell-model calculation, and the mirror nuclear structure in ^56Co. The associated uncertainties in the rates were estimated by a Monte Carlo method. Our revised rate is significantly different from the recent results, which were partially based on experimental results;in addition, we found that a result in a previous work was incorrect. We recommend our revised rate to be incorporated in the future astrophysical network calculations. | Shao-Bo Ma Li-Yong Zhang Jun Hu | 2019 | Nuclear Science and Techniques2019，30，9： | 0 |
| 4 | Effects of Microscopic Three-body Forces in Asymmetric Nuclear Matter显示文摘The efiects of microscopic three-body forces on the equatioil of state(EOS)and the single particle properties of isospin asymmetric nuclear matter have been studied within Brueckner-Hartree-Fock framework~[1]The microscopic three-body force model constructed from meson exchange current approach in Ref.~[2] has been extended to isospin asymmetric nuclear | Zuo Wi U.Lombardo A.Lejeune J.F.Mathiot | 2001 | IMP & HIRFL Annual Report2001，，1： | 0 |
| 5 | Study of Proton Resonances in ^(22)Mg by Resonant Elastic Scattering of ^(21)Na+p and Its Astrophysical Implication in ^(18)Ne(α,p) ^(21)Na Reaction Rate显示文摘Proton resonant states in 22Mg have been investigated by the resonant elastic scattering of 21Na+p. The 21Na beam with a mean energy of 4.00 MeV/u was separated by the CNS radioactive ion beam separator(CRIB) and bombarded a thick(CH2)n target. The energy spectra of recoiled protons were measured at scattering angles of θcm ≈172° and 146°,respectively. A new state at 7.06 MeV has been observed clearly and another new one at 7.28 MeV is tentatively identified due to its low statistics. The proton resonant parameters were deduced from an R-matrix analysis of the differential cross section data. The astrophysical resonant reaction rate for the 18Ne(α,p)21Na reaction has been estimated,and it is about five times larger than that assumed before. | S.Kubono T.Teranishi M.Notani H.Baba S.Nishimura J.Y.Moon M.Nishimura S.Michimasa H.Iwasaki Y.Yanagisawa N.Hokoiwa M.Kibe J.H.Lee S.Kato Y.Gono C.S.Lee | 2009 | 原子核物理评论2009，26，S1： | 0 |
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