A dynamic model of spherical perturbations in the Friedmann universe. I

DOI10.1007/s11182-008-9019-0zbMath1145.83363arXiv1101.1414OpenAlexW1971630025MaRDI QIDQ946699

Yu. G. Ignat'ev, N. El'makhi

Publication date: 24 September 2008

Published in: Russian Physics Journal (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1101.1414

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (3)

Evolution of spherical perturbations in the cosmological environment of degenerate scalar-charged fermions with a scalar Higgs coupling ⋮ Formation of supermassive nuclei of black holes in the early universe by the mechanism of scalar-gravitational instability. I: Local picture ⋮ The self-consistent field method and the macroscopic universe consisting of a fluid and black holes

Cites Work

• Spherically symmetric perturbation of an ultrarelativistic fluid in a homogeneous and isotropic universe
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