The radiative 10Be(n,g)11be capture at thermal and astrophysical energies

Abstract

Within the framework of the modified potential cluster model with the forbidden states and the classification of states according to Young tableaux the possibility of describing the available experimental data for the total reaction cross sections of the neutron radiative capture on 10Be at thermal and astrophysical energies was shown.

15p., 2 tabl., 4 fig., 62 ref. arXiv admin note: text overlap with arXiv:1506.07954

References in corpus (8)

• Nuclear Charge Radii of Be-7,9,10 and the one-neutron halo nucleus Be-11
• Astrophysical S-Factor of p2H Radiative Capture
• Thermonuclear Processes for Three Body System in the Potential Cluster Model
• 8li(n,g)9li reaction at superlow energies
• Radiative neutron capture on 9be, 14c, 14n, 15n and 16o at thermal and astrophysical energies
• Study of the neutron and proton capture reactions 10,11b(n, g), 11b(p, g), 14c(p, g), and 15n(p, g) at thermal and astrophysical energies
• Astrophysical S-factor of the radiative proton capture on 14C at low energies
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Cited by in corpus (7)

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• Study of the nucleon radiative captures 8Li(n,gamma)9Li, 9Be(p,gamma)10B, 10Be(n,gamma)11Be, 10B(p,gamma)11C, and 16O(p,gamma)17F at thermal and astrophysical energies
• New Results for the p7Be-->8Bgamma Astrophysical S-factor from 10 keV to 5 MeV and Reactions Rate from 0.01 to 10 T9
• Influence of low-lying resonances on reaction rates for n10B capture
• Influence of resonances on the 11B(n,gamma)12B capture reaction rate. Capture to the ground state of 12B
• New Results for Neutron Radiative Capture on 10be at Energies from 25.3 meV to 10.0 meV
• The radiative proton capture on 16O at astrophysical energies