Inflation cosmology with rotation with chaotic inflation
A cosmological scenario with rotation with a chaotic stage of inflation is constructed for the Bianchi type IX metric. Friedmann's stages of cosmology are described. It was found that in the modern era, the dark energy described by an anisotropic liquid practically does not rotate.
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Keywords
cosmological model, dark matter, dark energy, rotation of UniverseAuthors
| Name | Organization | |
| Panov V.F. | Perm State University | panov@psu.ru |
| Sandakova O.V. | Perm State University | o_sandakova@list.ru |
| Kuvshinova E.V. | Perm State University | kuvlenka@narod.ru |
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