Kinetic equations for ultrarelativistic particles in a Robertson-Walker Universe and isotropization of relict radiation by gravitational interactions
arXiv:1101.4303 · doi:10.1007/BF00639984
Abstract
Kinetic equations for ultrarelativistic particles with due account of gravitational interactions with massive particles in the Robertson-Walker universe are obtained. On the basis of an exact solution of the kinetic equations thus obtained, a conclusion is made as to the high degree of the uniformity of the relict radiation on scales with are less than .
19 pages, 2 figures, 13 references
Cited by in corpus (13)
- Cosmological Evolution of Statistical System of Scalar Charged Particles
- Statistical system with a fantom scalar interaction in the Gravitation Theory. I. The Microscopic Dynamics
- The cosmological evolution of the cosmological plasma with interpartial scalar interaction. I. The canonic formulation of classical scalar interaction
- Nonminimal Macroscopic Models of a Scalar Field Based on Microscopic Dynamics. I. Extension of the Theory for Negative Masses
- 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
- Spherically Symmetric Perturbation of Ultrarelativistic Fluid in Homogeneous and Isotropic Universe
- The Method of Self-Consistent Field and Macroscopical Einstein Equations for the Early Universe
- Dynamic model of spherical perturbations in the Friedmann universe. II. retarding solutions for the ultrarelativistic equation of state
- Formation of supermassive nuclei of Black holes in the early Universe by the mechanism of scalar-gravitational instability. III. Large scale picture
- Dynamic model of spherical perturbations in the Friedman universe. III. Automodel solutions
- Macroscopic Einstein Equations for a Cosmological Model with -term
- Statistical Cosmological Fermion Systems With Interparticle Fantom Scalar Interaction