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An Anisotropic Cosmological Model with Isotropic Background Radiation

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Current Trends in Relativistic Astrophysics

Part of the book series: Lecture Notes in Physics ((LNP,volume 617))

Abstract

We present an exact solution of Einstein equations that describes a Bianchi type III spacetime withconformal expansion. The matter content is given by an anisotropic scalar field and two perfect fluids representing dust and isotropic radiation. Based on this solution, we construct a cosmological model that respects the evolution of the scale factor predicted in standard cosmology.

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Authors and Affiliations

  1. I.M.A.F.F., C.S.I.C., Serrano 121, 28006, Madrid, Spain

    Saulo Carneiro & Guillermo A. Mena Marugán

  2. Instituto de Física, Universidade Federal da Bahia, 40210-340, Bahia, Salvador, Brazil

    Saulo Carneiro

Authors
  1. Saulo Carneiro
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  2. Guillermo A. Mena Marugán
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Editor information

Editors and Affiliations

  1. E.T.S.I.Navales, Universidad Politécnica de Madrid, Arco de la Victoria s/n, 28040, Madrid, Spain

    Leonardo Fernández-Jambrina

  2. Fac. Ciencias Físicas, Universidad Compluense de Madrid, Avenida Complutense s/n, 28040, Madrid, Spain

    Luis Manuel González-Romero

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© 2003 Springer-Verlag Berlin Heidelberg

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Carneiro, S., Marugán, G.A.M. (2003). An Anisotropic Cosmological Model with Isotropic Background Radiation. In: Fernández-Jambrina, L., González-Romero, L.M. (eds) Current Trends in Relativistic Astrophysics. Lecture Notes in Physics, vol 617. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-36973-2_17

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  • DOI: https://doi.org/10.1007/3-540-36973-2_17

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-01983-1

  • Online ISBN: 978-3-540-36973-8

  • eBook Packages: Springer Book Archive

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