THM determination of the 65 keV resonance strength intervening in the 17O(p,α)14N reaction rate

被引：0
作者：
Sergi, M. L. [1 ]
Spitaleri, C. [1 ,2 ]
Burjan, S. V. [3 ]
Cherubini, S. [1 ,2 ,4 ,5 ]
Coc, A.
Gulino, M. [1 ,2 ]
Hammache, F. [6 ,7 ]
Hons, Z.
Irgaziev, B. [8 ]
Kiss, G. G. [9 ]
Kroha, V. [3 ]
La Cognata, M. [1 ]
Lamia, L. [10 ]
Mukhamedzhanov, A. [11 ]
Pizzone, R. G. [1 ]
Puglia, S. M. R. [1 ,2 ]
Rapisarda, G. G. [1 ,2 ]
Romano, S. [1 ,2 ]
de Sereville, N. [12 ,13 ]
Somorjai, E. [9 ]
Tumino, A. [1 ,2 ]
机构：
[1] Ist Nazl Fis Nucl, Lab Nazl Sud, I-95129 Catania, Italy
[2] Univ Catania, Catania, Italy
[3] Nucl Phys Inst ASCR Rez Near Prague, Prague, Czech Republic
[4] CNRS, IN2P3, UMR 8609, CSNSM, F-91405 Orsay, France
[5] Univ Paris 11, F-91405 Orsay, France
[6] CNRS, IN2P3, IPN, F-91406 Orsay, France
[7] Univ Paris Sud, F-91406 Orsay, France
[8] GIK Inst Engn Sci & Technol Topi Dist Swabi NWFP, Peshawar, Pakistan
[9] ATOMKI, Debrecen, Hungary
[10] Univ Catania, Catania, Italy
[11] Texas A&M Univ, Inst Cyclotron, College Stn, TX 77843 USA
[12] CNRS, IN2P3, IPN, F-91406 Orsay, France
[13] Univ Paris 11, F-91406 Orsay, France
来源：
EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (V). FROM NUCLEI TO STARS | 2015年 / 1645卷
关键词：
Nuclear Astrophysics; Direct reactions; Nucleosynthesis in novae; supernovae; and other explosive environments; CROSS-SECTION; TROJAN; ALPHA)N-14; ENERGIES; O-18(P; O-17(P;
D O I：
10.1063/1.4909608
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The O-17(p,alpha)N-14 reaction is of paramount importance for the nucleosynthesis in a number of stellar sites, including red giants (RG), asymptotic giant branch (AGB) stars, massive stars and classical novae. We report on the indirect study of the O-17(p,alpha)N-14 reaction via the Trojan Horse Method by applying the approach recently developed for extracting the resonance strength of the narrow resonance at E-c.m.(R) = 65 keV (E-X = 5.673 MeV). The strength of the 65 keV resonance in the O-17(p,alpha)N-14 reaction, measured by means of the THM, has been used to renormalize the corresponding resonance strength in the O-17 + p radiative capture channel.
引用
收藏
页码：392 / 396
页数：5
相关论文
共 34 条
  • [1] Solar fusion cross sections. II. The pp chain and CNO cycles
    Adelberger, E. G.
    Garcia, A.
    Robertson, R. G. Hamish
    Snover, K. A.
    Balantekin, A. B.
    Heeger, K.
    Ramsey-Musolf, M. J.
    Bemmerer, D.
    Junghans, A.
    Bertulani, C. A.
    Chen, J. -W.
    Costantini, H.
    Prati, P.
    Couder, M.
    Uberseder, E.
    Wiescher, M.
    Cyburt, R.
    Davids, B.
    Freedman, S. J.
    Gai, M.
    Gazit, D.
    Gialanella, L.
    Imbriani, G.
    Greife, U.
    Hass, M.
    Haxton, W. C.
    Itahashi, T.
    Kubodera, K.
    Langanke, K.
    Leitner, D.
    Leitner, M.
    Vetter, P.
    Winslow, L.
    Marcucci, L. E.
    Motobayashi, T.
    Mukhamedzhanov, A.
    Tribble, R. E.
    Nollett, Kenneth M.
    Nunes, F. M.
    Park, T. -S.
    Parker, P. D.
    Schiavilla, R.
    Simpson, E. C.
    Spitaleri, C.
    Strieder, F.
    Trautvetter, H. -P.
    Suemmerer, K.
    Typel, S.
    [J]. REVIEWS OF MODERN PHYSICS, 2011, 83 (01) : 195 - 245
  • [2] A compilation of charged-particle induced thermonuclear reaction rates
    Angulo, C
    Arnould, M
    Rayet, M
    Descouvemont, P
    Baye, D
    Leclercq-Willain, C
    Coc, A
    Barhoumi, S
    Aguer, P
    Rolfs, C
    Kunz, R
    Hammer, JW
    Mayer, A
    Paradellis, T
    Kossionides, S
    Chronidou, C
    Spyrou, K
    Degl'Innocenti, S
    Fiorentini, G
    Ricci, B
    Zavatarelli, S
    Providencia, C
    Wolters, H
    Soares, J
    Grama, C
    Rahighi, J
    Shotter, A
    Rachti, ML
    [J]. NUCLEAR PHYSICS A, 1999, 656 (01) : 3 - 183
  • [3] COULOMB DISSOCIATION AS A SOURCE OF INFORMATION ON RADIATIVE-CAPTURE PROCESSES OF ASTROPHYSICAL INTEREST
    BAUR, G
    BERTULANI, CA
    REBEL, H
    [J]. NUCLEAR PHYSICS A, 1986, 458 (01) : 188 - 204
  • [4] MEASUREMENT OF THE O-17(P,ALPHA)N-14 CROSS-SECTION AT STELLAR ENERGIES
    BLACKMON, JC
    CHAMPAGNE, AE
    HOFSTEE, MA
    SMITH, MS
    DOWNING, RG
    LAMAZE, GP
    [J]. PHYSICAL REVIEW LETTERS, 1995, 74 (14) : 2642 - 2645
  • [5] Chafa A., 2000, PHYS REV C, V357, P561
  • [6] Indirect investigation of the d+Li-6 reaction at low energies relevant for nuclear astrophysics
    Cherubini, S
    Kondratyev, VN
    Lattuada, M
    Spitaleri, C
    Miljanic, D
    Zadro, M
    Baur, G
    [J]. ASTROPHYSICAL JOURNAL, 1996, 457 (02) : 855 - 858
  • [7] Coc A, 2000, ASTRON ASTROPHYS, V357, P561
  • [8] Explosive hydrogen burning of 17O in classical novae -: art. no. 081102
    Fox, C
    Iliadis, C
    Champagne, AE
    Coc, A
    José, J
    Longland, R
    Newton, J
    Pollanen, J
    Runkle, R
    [J]. PHYSICAL REVIEW LETTERS, 2004, 93 (08) : 081102 - 1
  • [9] Study of the 6Li(n, α)3H reaction via the 2H quasi-free break-up
    Gulino, M.
    Spitaleri, C.
    Cherubini, S.
    Crucilla, V.
    La Cognata, M.
    Lamia, L.
    Pizzone, R. G.
    Romano, S.
    Sergi, M. L.
    Tumino, A.
    Li Chengbo
    Elekes, Z.
    Somorjai, E.
    Burjan, V.
    Kroha, V.
    Mukhamedzhanov, A.
    [J]. JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, 2010, 37 (12)
  • [10] Charged-particle thermonuclear reaction rates: III. Nuclear physics input
    Iliadis, C.
    Longland, R.
    Champagne, A. E.
    Coc, A.
    [J]. NUCLEAR PHYSICS A, 2010, 841 : 251 - 322
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