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The continued interest to the study of the radiative neutron capture onatomic nuclei is caused, on the one hand, by the important role of this processin the analysis of many fundamental properties of nuclei and nuclear reactions,and, on the other hand, by the wide use of the capture cross section data inthe various applications of nuclear physics and nuclear astrophysics, and,also, by the analysis of the processes of primordial nucleosynthesis in theUniverse. This review is devoted to description of the results obtained for theprocesses of the radiative neutron capture at thermal and astrophysicalenergies on certain light atomic nuclei. The consideration of these processesis done in the frame of the potential cluster model, the general principles ofwhich and calculation methods were described earlier. The methods of usage ofthe obtained on the basis of the phase shift analysis intercluster potentialswill be directly demonstrated for calculations of the radiative capturecharacteristics. The considered capture reactions are not a part of stellarthermonuclear cycles, but they get in the basic reaction chain of primordialnucleosynthesis, taken place in the time of the Universe formation.

The radiative neutron capture on 2H, 6Li, 7Li, 12C and 13C at astrophysical energies