Bianchi Type VIII Cosmological Models Described with Caplygin Gas Equation of State Fluid Sources

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Within the general theory of relativity the Bianchi type VIII cosmological models with rotation and expansion have been built. It’s known that dark energy can be simulated by different kinds of energy-stress tensor, therefore the sources of gravitation in present article are an anisotropic fluid, with a pressure component satisfying to Chaplygin gas equation of state and a perfect fluid in the first case and an anisotropic fluid, Chaplygin gas and cosmological constant in the second case. It has been proved that the model, when expanding from Plank scale to the modern size gives satisfactory value of the angular velocity value. The found solutions can be used for effects taking place nowadays and at the inflationary stage.

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Daniil Yanishevskiy

Perm State University

编辑信件的主要联系方式.
Email: ydm86@yandex.ru

competitioner of Department of Higher Mathematics

15, Bukireva str., Perm, 614990, Russian Federation

参考

  1. K. Land, J. ao Magueijo, Examination of Evidence for a Preferred Axis in the Cosmic Radiation Anisotropy, Physical Review Letters 95 (2005) 071301–071304. doi: 10.1103/PhysRevLett.95.071301.
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  3. A. R. Liddle, M. Cortes, Cosmic Microwave Background Anomalies in an Open Universe, Physical Review Letters 111 (2013) 111302. doi: 10.1103/PhysRevLett.111.111302.
  4. G. M. Bradley, E. Sviestins, Some Rotating, Time-Dependent Bianchi Type VIII Cosmologies with Heat Flow, GRG 16 (1984) 1119–1133. doi: 10.1007/BF00760236.
  5. E. V. Kuvshinova, V. N. Pavelkin, V. F. Panov, O. V. Sandakova, Bianchi Type VIII Cosmological Models with Rotating Dark Energy, Gravitation and Cosmology 20 (2014) 141–143. doi: 10.1134/S0202289314020078.

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