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.
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USTHB, Fac Phys, BP 32, Algiers 16111, AlgeriaUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Belhout, A.
[1
]
Ouichaoui, S.
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USTHB, Fac Phys, BP 32, Algiers 16111, AlgeriaUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Ouichaoui, S.
[1
]
Beaumevieille, H.
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USTHB, Fac Phys, BP 32, Algiers 16111, AlgeriaUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Beaumevieille, H.
[1
]
Bouchemha, A.
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USTHB, Fac Phys, BP 32, Algiers 16111, AlgeriaUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Bouchemha, A.
[1
]
Bogaert, G.
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机构:
Univ Paris XI, CNRS, IN2P3, CSNSM, Campus Orsay, F-91405 Orsay, France
Univ Cote Azur, Artemis, CNRS, Observ Cote Azur, CS 34229, F-06304 Nice 4, FranceUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Bogaert, G.
[2
,4
]
Fortier, S.
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Univ Paris XI, CNRS, IN2P3, Inst Phys Nucl, F-91406 Orsay, FranceUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Fortier, S.
[3
]
Kiener, J.
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Univ Paris XI, CNRS, IN2P3, CSNSM, Campus Orsay, F-91405 Orsay, FranceUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Kiener, J.
[2
]
Lefebvre-Schuhl, A.
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Univ Paris XI, CNRS, IN2P3, CSNSM, Campus Orsay, F-91405 Orsay, FranceUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Lefebvre-Schuhl, A.
[2
]
Maison, J. M.
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Univ Paris XI, CNRS, IN2P3, Inst Phys Nucl, F-91406 Orsay, FranceUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Maison, J. M.
[3
]
Rosier, L.
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Univ Paris XI, CNRS, IN2P3, Inst Phys Nucl, F-91406 Orsay, FranceUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Rosier, L.
[3
]
Rotbard, J.
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Univ Paris XI, CNRS, IN2P3, Inst Phys Nucl, F-91406 Orsay, FranceUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Rotbard, J.
[3
]
Tatischeff, V.
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Univ Paris XI, CNRS, IN2P3, CSNSM, Campus Orsay, F-91405 Orsay, FranceUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Tatischeff, V.
[2
]
Thibaud, J. P.
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Univ Paris XI, CNRS, IN2P3, CSNSM, Campus Orsay, F-91405 Orsay, FranceUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
Thibaud, J. P.
[2
]
Vernotte, J.
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Univ Paris XI, CNRS, IN2P3, Inst Phys Nucl, F-91406 Orsay, FranceUSTHB, Fac Phys, BP 32, Algiers 16111, Algeria
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
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.