Model of the Origin of Cosmic Rays in the Galaxy

摘要

The origin of cosmic rays (CRs) is a key problem in astrophysics. As follows from the wide list of literature devoted to CR (see, e.g., reviews and monographs [1-3] and references to original studies therein), considerable progress has been achieved in understanding CR physics, although at present the process of CR generation is not completely understood. Therefore, constructing a model in which available experimental data are consistent with a reasonable theoretical substantiation of basic CR characteristics is rather urgent.