The 7Li (n,γ)8Li radiative capture at astrophysical energies

被引:34
|
作者
Dubovichenko, Sergey B. [1 ,2 ]
Dzhazairov-Kakhramanov, Albert V. [1 ]
机构
[1] Inst Nucl Phys NNC RK, Alma Ata 050032, Kazakhstan
[2] VG Fessenkov Astrophys Inst NCSRT NSA RK, Kamenskoe Plato 050020, Almaty, Kazakhstan
关键词
Neutron radiative capture process; primordial nucleosynthesis; nuclear astrophysics; cross sections; cluster model; phase shifts; S-FACTOR; LIGHT-NUCLEI; NEUTRON-CAPTURE; PROTON CAPTURE; CROSS-SECTIONS; P(13)C; (2)DE;
D O I
10.1002/andp.201200151
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The possibility to construct intercluster interaction potentials in continuous and discrete spectra is shown in one-channel cluster model based on the classification of orbital states according to Young schemes. These potentials usually contain Pauli forbidden states, and correctly describe elastic scattering phase shifts taking into account resonance behavior and main characteristics of the bound states of nuclei in the considering cluster channel. The versions of intercluster interaction potentials describing the resonance nature of some phase shifts of the n7Li elastic scattering at low energies and the P2 ground state of 8Li in the n7Li cluster channel have been constructed for the demonstration of this approach. The possibility of describing the total cross sections of 7Li (n,?)8Li within the energies from 5 meV (5 center dot 10-3 eV) to 1 MeV, including resonance at 0.25 MeV, has been demonstrated for the potentials obtained in the potential cluster model with forbidden states.
引用
收藏
页码:850 / 861
页数:12
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