New determination of proton spectroscopic factors and reduced widths for 8Be states in the 16.5-18.0 MeV excitation energy region via the study of the 7Li(3He, d)8Be transfer reaction at Elab=20 MeV: Implication for the 7Li(p, α)4He hydrogen burning reaction

被引:4
作者
Belhout, A. [1 ]
Ouichaoui, S. [1 ]
Beaumevieille, H. [1 ]
Bouchemha, A. [1 ]
Bogaert, G. [2 ,4 ]
Fortier, S. [3 ]
Kiener, J. [2 ]
Lefebvre-Schuhl, A. [2 ]
Maison, J. M. [3 ]
Rosier, L. [3 ]
Rotbard, J. [3 ]
Tatischeff, V. [2 ]
Thibaud, J. P. [2 ]
Vernotte, J. [3 ]
机构
[1] USTHB, Fac Phys, BP 32, Algiers 16111, Algeria
[2] Univ Paris XI, CNRS, IN2P3, CSNSM, Campus Orsay, F-91405 Orsay, France
[3] Univ Paris XI, CNRS, IN2P3, Inst Phys Nucl, F-91406 Orsay, France
[4] Univ Cote Azur, Artemis, CNRS, Observ Cote Azur, CS 34229, F-06304 Nice 4, France
关键词
LIGHT-NUCLEI; CROSS-SECTION; P; D REACTIONS; HE-3; NUCLEOSYNTHESIS; SCATTERING; MECHANISM; 6LI;
D O I
10.1103/PhysRevC.96.054601
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The angular distributions of Be-8 states in the excitation energy region E-x similar to (16.5-18.2) MeV produced in the Li-7(He-3, d)Be-8 proton transfer reaction have been measured at the Orsay 14.8-MV tandem accelerator for He-3(2+) ion bombarding energy, E-lab = 20 MeV, and forward angular range, theta(lab) = 5 degrees-50 degrees. A high energy resolution detection system composed of a split-pole magnetic spectrometer and a Delta E - E, position-sensitive drift chamber was used to record the energy spectra of outgoing deuterons. The measured cross section data for the direct reaction component have been separated from the compound nucleus one, then analyzed in the framework of the nonlocal, finite-range (FR)-distorted-wave Born approximation (DWBA) theory. New values of the (CS)-S-2 and (Sp(1/2), S-p3/2) proton absolute and partial spectroscopic factors and related gamma(2)(p)(a) proton reduced widths versus the p + Li-7 channel radius have been extracted for the 2(+)(16.626) and 2(+)(16.922), T = 0 + 1 isospin-mixed loosely bound states of astrophysical interest and the 1(+)(17.640), T = 1 unbound state of Be-8. They are compared to sparse earlier experimental values and to shell-model-predicted ones from the literature, and are discussed. In particular, the status of the spectroscopic information on the 2(+) isospin-mixed doublet is reviewed and updated. The application in nuclear astrophysics of the DWBA derived results is emphasized.
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页数:13
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共 97 条
  • [1] Solar fusion cross sections
    Adelberger, EG
    Austin, SM
    Bahcall, JN
    Balantekin, AB
    Bogaert, G
    Brown, LS
    Buchmann, L
    Cecil, FE
    Champagne, AE
    de Braeckeleer, L
    Duba, CA
    Elliott, SR
    Freedman, SJ
    Gai, M
    Goldring, G
    Gould, CR
    Gruzinov, A
    Haxton, WC
    Heeger, KM
    Henley, E
    Johnson, CW
    Kamionkowski, M
    Kavanagh, RW
    Koonin, SE
    Kubodera, K
    Langanke, K
    Motobayashi, T
    Pandharipande, V
    Parker, P
    Robertson, RGH
    Rolfs, C
    Sawyer, RF
    Shaviv, N
    Shoppa, TD
    Snover, KA
    Swanson, E
    Tribble, RE
    Turck-Chieze, S
    Wilkerson, JF
    [J]. REVIEWS OF MODERN PHYSICS, 1998, 70 (04) : 1265 - 1291
  • [2] BRUSLIB and NETGEN: the Brussels nuclear reaction rate library and nuclear network generator for astrophysics
    Aikawa, M
    Arnould, M
    Goriely, S
    Jorissen, A
    Takahashi, K
    [J]. ASTRONOMY & ASTROPHYSICS, 2005, 441 (03) : 1195 - 1203
  • [3] ENERGY-LEVELS OF LIGHT-NUCLEI A=5-10
    AJZENBERGSELOVE, F
    [J]. NUCLEAR PHYSICS A, 1984, 413 (01) : 1 - 214
  • [4] ENERGY-LEVELS OF LIGHT-NUCLEI A = 5-10
    AJZENBERGSELOVE, F
    [J]. NUCLEAR PHYSICS A, 1988, 490 (01) : 1 - 225
  • [5] First Direct Measurement of the 2H(α,γ)6Li Cross Section at Big Bang Energies and the Primordial Lithium Problem
    Anders, M.
    Trezzi, D.
    Menegazzo, R.
    Aliotta, M.
    Bellini, A.
    Bemmerer, D.
    Broggini, C.
    Caciolli, A.
    Corvisiero, P.
    Costantini, H.
    Davinson, T.
    Elekes, Z.
    Erhard, M.
    Formicola, A.
    Fueloep, Zs.
    Gervino, G.
    Guglielmetti, A.
    Gustavino, C.
    Gyuerky, Gy.
    Junker, M.
    Lemut, A.
    Marta, M.
    Mazzocchi, C.
    Prati, P.
    Alvarez, C. Rossi
    Scott, D. A.
    Somorjai, E.
    Straniero, O.
    Szuecs, T.
    [J]. PHYSICAL REVIEW LETTERS, 2014, 113 (04)
  • [6] 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
  • [7] Lithium isotopic abundances in metal-poor halo stars
    Asplund, Martin
    Lambert, David L.
    Nissen, Poul Erik
    Primas, Francesca
    Smith, Verne V.
    [J]. ASTROPHYSICAL JOURNAL, 2006, 644 (01) : 229 - 259
  • [8] STANDARD SOLAR MODELS, WITH AND WITHOUT HELIUM DIFFUSION, AND THE SOLAR NEUTRINO PROBLEM
    BAHCALL, JN
    PINSONNEAULT, MH
    [J]. REVIEWS OF MODERN PHYSICS, 1992, 64 (04) : 885 - 926
  • [9] ISOSPIN MIXING IN LIGHT-NUCLEI
    BARKER, FC
    [J]. AUSTRALIAN JOURNAL OF PHYSICS, 1978, 31 (01): : 27 - 45
  • [10] INTERMEDIATE COUPLING SHELL-MODEL CALCULATIONS FOR LIGHT NUCLEI
    BARKER, FC
    [J]. NUCLEAR PHYSICS, 1966, 83 (02): : 418 - &