Thermonuclear Processes for Three Body System in the Potential Cluster Model

Abstract

The manuscript is devoted to the description of the results obtained in the frame of the modified potential cluster model with the classification of states according to Young tableaux for neutron and proton radiative capture processes on 2H at thermal and astrophysical energies. It demonstrates methods of application that were obtained on the basis of phase shift analysis and characteristics of the bound states of 2H potentials for consideration of the radiative capture processes. First reaction of the proton capture directly takes part in the pp solar cycle, where it is the second reaction. The neutron capture is not a part of usual thermonuclear cycles in the Sun and stars, but can take part in the processes of primordial nucleosynthesis, following at formation and evolution of our entire Universe.

arXiv admin note: text overlap with arXiv:1202.1995

References in corpus (6)

• 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
• Astrophysical S-factor of the radiative proton capture on 14C at low energies
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Cited by in corpus (16)

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• The ${}^6$Li$(p,\gamma {)}^7$Be reaction rate in the light of the new LUNA data
• 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
• New results for radiative 3He(2H,gamma)5Li capture at astrophysical energy and its possible role in accumulation of 6Li at the BBN
• 12B(n,gamma)13B reaction as alternative path to astrophysical synthesis of 13C isotope
• 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
• Reanalysis of ${}^{13}$N($p,\gamma$)${}^{14}$O reaction and its role in stellar CNO cycle
• Radiative 3He(2H,g)5Li capture at low deuterium energy
• The comparative role of 7Li(n,γ) reaction in primordial nucleosynthesis