Dynamic model of spherical perturbations in the Friedman universe. III. Automodel solutions

Abstract

A class of exact spherically symmetric perturbations of retarding automodel solutions linearized around Friedman background of Einstein equations for an ideal fluid with an arbitrary barotrope value is obtained and investigated.

arXiv comment12 pages, 4 figures, 8 references

References in corpus (2)

• Kinetic equations for ultrarelativistic particles in a Robertson-Walker Universe and isotropization of relict radiation by gravitational interactions
• Spherically Symmetric Perturbation of Ultrarelativistic Fluid in Homogeneous and Isotropic Universe

Cited by in corpus (2)

• Evolution of spherical perturbations in the cosmological environment of degenerate scalarly charged fermions with the Higgs scalar interaction
• Formation of supermassive nuclei of Black holes in the early Universe by the mechanism of scalar-gravitational instability. I. Local picture