Nuclear Structure Aspects in Nuclear Astrophysics

Michael S.Smith

近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。

本刊再次郑重声明：

（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137

（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。

（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。

《中国物理C》（英文）编辑部

2024年10月30日

Chinese Physics C> 2006, Vol. 30> Issue(S2) : 214-218

Nuclear Structure Aspects in Nuclear Astrophysics

Michael S.Smith

Physics Division,Oak Ridge National Laboratory,Oak Ridge,TN,37831-6354,USA

Abstract
HTML
Reference
Related

PDF

Abstract：
Nuclear structure information plays an extremely important role in studies of the evolution and explosion of stars and the cosmic synthesis of the elements. Properties of nuclear ground states (e.g., masses, lifetimes, decay branches) and low-lying resonances (excitation energies, spins, parities, decay widths, spectroscopic factors), especially on unstable nuclei, can quantitatively and qualitatively change predictions of astrophysical simulations. The location of the particle driplines and shell structure far from stability also strongly influence our astrophysical predictions. A number of examples of the dramatic impact that new nuclear structure information has on simulations of nova explosions, X-ray bursts, and core collapse supernovae are given. Some of these are results of recent measurements with radioactive ¹⁸F, ⁸²Ge, and ⁸⁴Se beams at ORNL's Holifield Radioactive Ion Beam Facility. A new suite of software tools to help determine the astrophysical impact of nuclear physics studies will also be presented.

[1]	LIU Ying , LIANG Nai-Li , LI Ming-Fei , ZHU Li-Hua , WU Xiao-Guang , HE Chuang-Ye , CUI Xing-Zhu , LI Li-Hua , WANG Zhi-Min , LI Guang-Sheng , WEN Shu-Xian , HUO Jun-De , YANG Ch . Level Structure of ¹⁵⁵Tm. Chinese Physics C, 2006, 30(S2): 160-162.
[2]	XU Yi , XU Wang , MA Yu-Gang , CAI Xiang-Zhou , CHEN Jin-Gen , GU Jia-Hui , GUO Wei , PAN Qiang-Yan , SHEN Wen-Qing , WANG Cheng-Bin , WANG Hong-Wei , XU Jia-Qiang , YUAN Ren-Yong . Study on the Reaction Rate of Key Reaction $\bf ^{12}$C($\bm\upalpha$,~$\bm\upgamma$)$\bf ^{16}$O in Astrophysics Base on Shanghai Laser Electron $\bm\upgamma$ Source. Chinese Physics C, 2006, 30(S2): 252-254.
[3]	ZHOU Wen-Ping , ZHAO Yan-Xin , ZHAO Guang-Yi , MA Ying-Jun , LU Jing-Bin , WANG Shou-Yu , SUN Liang , YANG Dong , LI Xian-Feng , MA Chun-Hui , LIU Yun-Zuo , ZHU Li-Hua , WU Xiao-Gu , , , . New Band Structures and Electromagnetic Properties in ¹⁵⁸Tm. Chinese Physics C, 2006, 30(S2): 151-153.
[4]	ZHU Sheng-Yun¹ , ZHOU Dong-Mei¹ , YUAN Da-Qing¹ , ZHENG Yong-Nan¹ , ZUO Yi¹ , LUO Qi¹ , ZHU Jia-Zheng¹ , XU Yong-Jun¹ , LI Guang-Sheng¹ , WU Xiao-Guan¹ , ZHU Li-Hua¹ , LI An-Li¹ , LIU Meng<sup , , , . Nuclear Moment Measurements and Nuclear Structure Studies. Chinese Physics C, 2006, 30(S2): 146-150.
[5]	XING Yong-Zhong , LIU Jian-Ye , ZUO Wei , LI Xi-Guo . Special Role of Neutron-Halo Nucleus on the Momentum Dissipation in Heavy Ion Collisions. Chinese Physics C, 2005, 29(10): 978-982.
[6]	LIU Jian-Ye , GUO Wen-Jun , REN Zhong-Zhou , XING Yong-Zhong , ZUO Wei , LI Xi-Guo . Special Role of Neutron-Halo Structure in the Fragmentation Reactions. Chinese Physics C, 2005, 29(8): 761-765.
[7]	SU Zong-Di , ZHOU Jian-Ming , WANG Bin , FENG Reng-Fa , WANG Shu-Nuan , SHI Shu-Mei , DAI Neng-Xiong , WANG Yu-Sheng , ZHU Yao-Yin , LI Zhi-Wen , LI Ming-Fei , LIU Jian-Feng , , . Nuclear Structure Database(NSDB). Chinese Physics C, 2004, 28(S1): 96-98.
[8]	CHEN Yong-Shou , SHU Neng-Chuan , WU Kai-Su . Explosive Nucleosynthesis in Astrophysics. Chinese Physics C, 2004, 28(12): 1349-1355.
[9]	PENG Qiu-He . Where Do the Extra High Energy Cosmic Rays Come From A Model of Active Galactic Nuclei With Magnetic Monopoles. Chinese Physics C, 2002, 26(S1): 104-111.
[10]	YU Lei , LIU Shu-Xin , LEI Yi-An , ZENG Jin-Yan . Underlying Physics of Identical Odd-and Even-Mass Bands in Normally Deformed Rare-Earth Nuclei. Chinese Physics C, 2001, 25(6): 526-532.
[11]	CHEN Yong-Shou . New Opportunities of Nuclear Structure. Chinese Physics C, 2000, 24(S1): 1-5.
[12]	LIU Wei-Ping , BAI Xi-Xiang , WANG You-Bao , LI Zhi-Hong , LIAN Gang , LI Zhi-Chang , GUO Gang , JIANG Li-Yang , LU Shao-Jun , FU Chang-Bo , CHEN Yong-Shou . Study of Astrophysical Nuclear Reaction on Beijing Secondary Beam Line GIRAFFE. Chinese Physics C, 2000, 24(S1): 6-8.
[13]	Bai Xinhua , Hu Jimin . Microscopic Calculations of Light Nuclei Structure. Chinese Physics C, 1997, 21(3): 235-247.
[14]	Liu Hang , Liu Jianye , Li Junqing . Study of the Structure Effect in Fragment Formation Process in HIC. Chinese Physics C, 1996, 20(8): 723-728.
[15]	ZHENG Ren-Rong , ZHU Shun-Quan . EFV APPROACH TO MICROSCOPIC NUCLEAR STRUCTURE. Chinese Physics C, 1990, 14(12): 1088-1095.
[16]	LIU Jian-Ye , TAN Nan-Hong , QIAO Wei-Min . THE ROLE OF NUCLEAR STRUCTURE EFFECTS ON THE NUCLEON EXCHANGE PROCESS IN DISSIPATIVE HEAVY-ION COLLISIONS. Chinese Physics C, 1989, 13(11): 1032-1038.
[17]	KONG Fan-Xin , LIU Ji-Feng , LIU Yuan . INFLUENCE OF NUCLEAR STRUCTURE OF He⁴ ON He⁴-NUCLEUS COLLISIONS AT HIGH ENERGIES. Chinese Physics C, 1984, 8(6): 707-711.
[18]	LI YANG-GUO , WU ZONG-EN , HUANG CHAO-HUI , LI YANG-GHO . π-NUCLEAR DOUBLE CHARGE EXCHANGE REACTION AND NUCLEAR STRUCTURE. Chinese Physics C, 1981, 5(2): 157-168.
[19]	Liu Xian-hui , Wu Zong-en , Huang Chao-hui , Li Yang-guo . π-NUCLEAR DOUBLE CHARGE EXCHANGE REACTION AND NUCLEAR STRUCTURE. Chinese Physics C, 1980, 4(3): 394-397.
[20]	R.L.Robinson , A.V.Ramayya . DISCOVERY OF MULTIPLE,COLLECTIVE BAND STRUCTURES IN NUCLEI WITH A=60—80. Chinese Physics C, 1979, 3(3): 355-381.

Access

Get Citation

Michael S.Smith. Nuclear Structure Aspects in Nuclear Astrophysics[J]. Chinese Physics C, 2006, 30(S2): 214-218.

Michael S.Smith. Nuclear Structure Aspects in Nuclear Astrophysics[J]. Chinese Physics C, 2006, 30(S2): 214-218. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2006-10-18
Revised: 1900-01-01

Article Metric

Article Views(4065)
PDF Downloads(588)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

Nuclear Structure Aspects in Nuclear Astrophysics

Michael S.Smith

Physics Division,Oak Ridge National Laboratory,Oak Ridge,TN,37831-6354,USA

Received Date: 2006-10-18
Accepted Date: 1900-01-01
Available Online: 2006-01-03

Abstract: Nuclear structure information plays an extremely important role in studies of the evolution and explosion of stars and the cosmic synthesis of the elements. Properties of nuclear ground states (e.g., masses, lifetimes, decay branches) and low-lying resonances (excitation energies, spins, parities, decay widths, spectroscopic factors), especially on unstable nuclei, can quantitatively and qualitatively change predictions of astrophysical simulations. The location of the particle driplines and shell structure far from stability also strongly influence our astrophysical predictions. A number of examples of the dramatic impact that new nuclear structure information has on simulations of nova explosions, X-ray bursts, and core collapse supernovae are given. Some of these are results of recent measurements with radioactive ¹⁸F, ⁸²Ge, and ⁸⁴Se beams at ORNL's Holifield Radioactive Ion Beam Facility. A new suite of software tools to help determine the astrophysical impact of nuclear physics studies will also be presented.