Cosmological models with Bianchi type V metric
Within the framework of General relativity, two cosmological models are constructed for a type V metric according to the Bianchi classification. In the first model, an anisotropic liquid is used as the source of gravity. This model is non-stationary and non-rotating. In the second cosmological model, anisotropic liquid and pure radiation are used as sources of gravity. All kinematic parameters of the models are found. Both models are examined for causality.
Download file
Counter downloads: 30
Keywords
cosmological model, Einstein equations, dark energyAuthors
Name | Organization | |
Kuvshinova E.V. | Perm State University | kuvlenka@narod.ru |
Sandakova O.V. | Perm State Agro-Technological University named after Academician D.N. Pryanishnikov | o_sandakova@list.ru |
Yanishevsky D.M. | Perm State University | ydm86@yandex.ru |
References
Короткий В.А. Релятивистская космология с вращением: дис. … канд. физ.-мат. наук. - М.: МГУ, 1987.
Гуц А.К. // Изв. вузов. Физика. - 1980. - Т. 23. - № 6. - С. 109-110.
Raval H.M. // Austral. J. Phys. - 1967. - V. 20. - Nо. 6. - P.663-673.
Агаков В.Г. // Вестник МГУ. Сер. 3. Физика. Астрономия. - 1979. - Т. 20. - № 4. - С. 73-80.
Agakov V.G. // Gen. Relativ. Gravit. - 1984. - V. 16. - No. 4. - P. 317-323.
