Pages that link to "Item:Q946699"
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The following pages link to A dynamic model of spherical perturbations in the Friedmann universe. I (Q946699):
Displaying 12 items.
- Spherically symmetric perturbations of spatially flat Friedmann models with imperfect fluid (Q954178) (← links)
- A dynamic model of spherical perturbations in the Friedmann universe. III. Self-similar solutions (Q1033697) (← links)
- The development of perturbations in the universe described by the nonstationary equation of state (Q1048629) (← links)
- The development of perturbations in the Universe described by the nonstationary equation of state (Q1049334) (← links)
- Spherically symmetric cosmological perturbation in a universe with background field (Q1384922) (← links)
- The self-consistent field method and the macroscopic universe consisting of a fluid and black holes (Q2303638) (← links)
- A dynamic model of spherical perturbations in the Friedmann universe. II: Retarded solutions to an ultrarelativistic equation of state (Q2380132) (← links)
- Analytical perfect fluid perturbation for the matter dominated epoch (Q2487223) (← links)
- (Q3219176) (← links)
- Evolution of spherical perturbations in the cosmological environment of degenerate scalar-charged fermions with a scalar Higgs coupling (Q6167606) (← links)
- Formation of supermassive nuclei of black holes in the early universe by the mechanism of scalar-gravitational instability. I: Local picture (Q6204645) (← links)
- Formation of supermassive nuclei of black holes in the early universe by the mechanism of scalar-gravitational instability. III: Large-scale picture (Q6579453) (← links)