2013/10/01 by Sergey Dubovichenko, SERGEY DUBOVICHENKO, Albert Dzhazairov-Kakhramanov +3
Physics and Astronomy · #Astronomical and nuclear sciences #Big Bang nucleosynthesis #Neutron #Neutron capture #Nuclear astrophysics #Nuclear physics research studies #Nuclear reaction #Nucleosynthesis #Quantum Chromodynamics and Particle Interactions #Radiative transfer #Thermonuclear fusion #nucl-th
paper · pdf · doi:10.1142/s0218301313500754
published as Int. J. of Mod. Phys. E Vol. 22 (2013) 1350075 · 50p., 122 Refs., 1 Tab., 10 Fig. arXiv admin note: text overlap with arXiv:1311.5284, arXiv:1212.1765, arXiv:1311.5295, arXiv:1304.1976
openalex publication_date 2013/10/01 · arxiv created 2014/01/28 · arxiv updated 2014/01/29 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The total cross-sections of the radiative neutron capture processes on 9 Be , 14 C , 14 N , 15 N and 16 O are described in the framework of the modified potential cluster model with the classification of orbital states according to Young tableaux. The continued interest in the study of these reactions is due, on the one hand, to the important role played by this process in the analysis of many fundamental properties of nuclei and nuclear reactions, and, on the other hand, to the wide use of the capture cross-section data in the various applications of nuclear physics and nuclear astrophysics, and, also, to the importance of the analysis of primordial nucleosynthesis in the Universe. This article is devoted to the description of results for the processes of the radiative neutron capture on certain light atomic nuclei at thermal and astrophysical energies. The considered capture reactions are not part of stellar thermonuclear cycles, but involve in the reaction chains of inhomogeneous Big Bang models.