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Cosmological solution of the Einstein—Weyl equation

  • Physics of Elementary Particles and Field Theory
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Russian Physics Journal Aims and scope

Abstract

The accurate integration of the Einstein—Weyl field equations is considered for the case when the spinor field depends only on the time, while the metric specifies a uniform space—time of type I in the Bianci classification, i.e., a particular case of a Steckel space of type (3.0).

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Authors
  1. A. N. Makarenko
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  2. V. V. Obukhov
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Additional information

Tomsk State Pedagogical University. Tomsk State University. Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 11, pp. 69–78, November, 1998.

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Makarenko, A.N., Obukhov, V.V. Cosmological solution of the Einstein—Weyl equation. Russ Phys J 41, 1124–1133 (1998). https://doi.org/10.1007/BF02514491

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  • DOI: https://doi.org/10.1007/BF02514491

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