A BRIEF ANALYSIS OF THE NEW SOLUTIONS OBTAINED FOR THE GRAVITY FIELD ON THE BASIS OF SCALAR-TENSOR THEORY

Abstract

This article shows the possibilities of using the scalar-tensor theory in finding the kinetic coupling function  and potential  of the non-singular static spherical-symmetric metric. In this case, it is taken into account that the scalar field can change its state from canonical to phantom in certain coordinates. The appearance of STN is determined by the Simpson-Visser metric, not in the full area of the radial coordinate, but in a limited area.