Astrophysical S-Factors and Reaction Rates of Threshold (p,n)-Reactions on 99-102Ru

被引：0
作者：
Skakun, Ye [1 ]
Rauscher, T. [2 ]
机构：
[1] Kharkiv Inst Phys & Technol, Natl Sci Ctr, Acad Skaja Str 1, UA-61108 Kharkov, Ukraine
[2] Univ Basel, Dept Phys, CH-4056 Basel, Switzerland
来源：
10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES | 2010年 / 1269卷
关键词：
(p; n); reactions; statistical model; reaction rates; p-process; nucleosynthesis; CAPTURE CROSS-SECTIONS; PROCESS NUCLEOSYNTHESIS; NUCLEAR ASTROPHYSICS; GAMMA-PROCESSES; P-PROCESS; RELEVANT; MODEL;
D O I：
10.1063/1.3485176
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Astrophysical S-factors of (p,n) reactions on Ru-99, Ru-100, Ru-101, and Ru-102 were derived from the sum of experimental isomeric and ground states cross sections measured in the incident proton energy range of 5-9 MeV. They were compared with Hauser-Feshbach statistical model predictions of the NON-SMOKER code. Good agreement was found in the majority of cases. Reaction rates were derived up to 8.7 GK stellar temperature by combining experiment and theory.
引用
收藏
页码：390 / +
页数：2
相关论文
共 15 条
  • [1] Experimental astrophysical reaction rates of threshold (p,n)-reactions on Pd isotopes
    Skakun, Ye.
    Rauscher, T.
    ORIGIN OF MATTER AND EVOLUTION OF GALAXIES, 2008, 1016 : 439 - +
  • [2] Theoretical exploration of S-factors for nuclear reactions of astrophysical importance
    Singh, Vinay
    Lahiri, Joydev
    Basu, D. N.
    NUCLEAR PHYSICS A, 2019, 987 : 260 - 273
  • [3] Calculations of Cross-Sections and Astrophysical S-factors for the (α,n) Reactions of Some Structural Fusion Materials
    Yildiz, Ercan
    Aydin, Abdullah
    Sarpun, Ismail Hakki
    Tel, Eyyup
    JOURNAL OF FUSION ENERGY, 2017, 36 (4-5) : 149 - 151
  • [4] Indirect Measurement of Astrophysical 13C(α, n)16O S-Factors
    Guo Bing
    Li Zhihong
    Li Yunju
    Su Jun
    Bai Xixiang
    Chen Yongshou
    Fan Qiwen
    Jin Sunjun
    Li Ertao
    Li Zhichang
    Lian Gang
    Liu Xin
    Liu Jiancheng
    Shu Nengchuan
    Wang Baoxiang
    Wang Youbao
    Yan Shengquan
    Zeng Sheng
    Liu Weiping
    Pang Danyang
    Lugaro, M.
    Buntain, J.
    PLASMA SCIENCE & TECHNOLOGY, 2012, 14 (05) : 357 - 359
  • [5] Astrophysical S-factors, Thermonuclear Rates, and Electron Screening Potential for the 3He(d,p)4He Big Bang Reaction via a Hierarchical Bayesian Model
    de Souza, Rafael S.
    Iliadis, Christian
    Coc, Alain
    ASTROPHYSICAL JOURNAL, 2019, 872 (01)
  • [6] Determination of the Astrophysical S(E) Factors or Rates for Radiative Capture Reaction with One Nucleon Transfer Reaction
    李志宏
    郭冰
    李云居
    苏俊
    李二涛
    白希祥
    王友宝
    曾晟
    王宝祥
    颜胜权
    李志常
    刘建成
    连钢
    金孙均
    刘鑫
    柳卫平
    Plasma Science and Technology, 2012, 14 (06) : 488 - 491
  • [7] Determination of the Astrophysical S(E) Factors or Rates for Radiative Capture Reaction with One Nucleon Transfer Reaction
    Li Zhihong
    Guo Bing
    Li Yunju
    Su Jun
    Li Ertao
    Bai Xixiang
    Wang Youbao
    Zeng Sheng
    Wang Baoxiang
    Yan Shengquan
    Li Zhichang
    Liu Jiancheng
    Lian Gang
    Jin Sunjun
    Liu Xin
    Liu Weiping
    PLASMA SCIENCE & TECHNOLOGY, 2012, 14 (06)
  • [8] Extrapolation of Astrophysical S Factors for the Reaction 14N(p,γ)15O to Near-Zero Energies
    Artemov, S. V.
    Igamov, S. B.
    Tursunmakhatov, Q. I.
    Yarmukhamedov, R.
    PHYSICS OF ATOMIC NUCLEI, 2012, 75 (03) : 291 - 309
  • [9] 12C(20Ne, 16O)16O α-transfer reaction and astrophysical S-factors at 300 keV
    Mondal, Ashok Kumar
    Basu, C.
    Adhikari, S.
    Bhattacharya, C.
    Rana, T. K.
    Kundu, S.
    Manna, S.
    Pandey, R.
    Roy, P.
    Sen, A.
    Meena, J. K.
    Saha, A. K.
    Sahoo, J. K.
    Basak, Dipali
    Bar, Tanmay
    Pai, Haridas
    Bisoi, A.
    Mitra, A. K.
    Biswas, Piyasi
    INTERNATIONAL JOURNAL OF MODERN PHYSICS E, 2021, 30 (05):
  • [10] DETERMINATION OF THE CL-35(N, P)S-35 REACTION CROSS-SECTION AND ITS ASTROPHYSICAL IMPLICATIONS
    DRUYTS, S
    WAGEMANS, C
    GELTENBORT, P
    NUCLEAR PHYSICS A, 1994, 573 (02) : 291 - 305
12