8li(n,g)9li reaction at superlow energies
arXiv:1506.07954 · doi:10.3847/0004-637X/819/1/78
Abstract
Within the framework of the modified potential cluster model with the state classification of nuclear particles according to Young tableaux the possibility of describing the available experimental data for the total cross sections of the neutron radiative capture on 8Li at thermal and astrophysical energies was considered.
19p., 1 tabl., 5 fig
References in corpus (5)
- Astrophysical S-Factor of p2H Radiative Capture
- 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
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- New Results for the p7Be-->8Bgamma Astrophysical S-factor from 10 keV to 5 MeV and Reactions Rate from 0.01 to 10 T9
- New Theoretical Results for Radiative 3H(p, γ)4He, 3He(2H, γ)5Li, 4He(2H, γ)6Li, 4He(3H, γ)7Li, and 4He(3He, γ)7Be Captures At Astrophysical Energies
- 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
- The radiative 10Be(n,g)11be capture at thermal and astrophysical energies
- New Results for Neutron Radiative Capture on 10be at Energies from 25.3 meV to 10.0 meV
- Gamow shell model description of the radiative capture reaction LiLi
- New results for radiative 3He(2H,gamma)5Li capture at astrophysical energy and its possible role in accumulation of 6Li at the BBN
- Role of resonances in the 8li(p,g)9be capture on reaction rate of the relevant astrophysical synthesis of 9be
- Reaction Rate Of p14N --> 15Ogamma Capture To All Bound States In Potential Cluster Model
- Radiative 3He(2H,g)5Li capture at low deuterium energy
- The radiative proton capture on 16O at astrophysical energies
- The comparative role of 7Li(n,γ) reaction in primordial nucleosynthesis