  The book covers the certain questions of nuclear physics and nuclear
astrophysics of light atomic nuclei and their processes at low and ultralow
energies. Some methods of calculation of nuclear characteristics of the
thermonuclear processes considered in nuclear astrophysics are given here. The
obtained results are directly applicable to the solution of certain nuclear
astrophysics problems in the field of description of the thermonuclear
processes in the Sun, the stars and the Universe. The book is based on the
results of approximately three-four tens of scientific papers generally
published in recent five-seven years and consists of three sections. The first
of them covers the description of the general methods of calculation of certain
nuclear characteristics for the bound states or the continuum of quantum
particles. The second section deals with the methods, the computer programs and
the results of the phase shift analysis of elastic scattering in the p3He,
p6Li, p12C, n12C, p13C, 4He4He and 4He12C nuclear systems at low and ultralow
energies. The results obtained on the basis of three-body models of certain
light atomic nuclei are given in the third section, notably the 7Li, 9Be and
11B nuclei which are used for examination of the conjugated intercluster
potentials determined on the basis of the phase shifts of elastic scattering
and using then in the nuclear astrophysics problems connected with the
description of the thermonuclear processes in the Universe. The book will be
useful for advanced students, postgraduate students and PhD doctoral candidates
in universities and research institutes in the field of astrophysics and
nuclear physics. The book is presented in Russian with a few inserts into
English.
