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Strong gravitational waves in semiclosed electromagnetic universes. Complete system of Newman-Penrose equations and radial dependence of the field variables

  • Elementary Particle Physics and Field Theory
  • Published:
Soviet Physics Journal Aims and scope

Abstract

We consider the process of integration of a complete system of Newman-Penrose equations for electrovacuum spaces of the general theory of relativity with nonzero cosmological constant. The restrictions used for the field variables correspond to strong gravitational waves in semiclosed Universes of Bertotti-Robinson type.

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Literature cited

  1. V. I. Khlebnikov, Izv. Vyssh. Uchebn. Zav., Fiz., No. 11, 74 (1987).

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Authors and Affiliations

  1. Institute of Problems in Mechanics, Academy of Sciences of the USSR, USSR

    V. I. Khlebnikov

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  1. V. I. Khlebnikov
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 12, pp. 29–33, December, 1987.

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Khlebnikov, V.I. Strong gravitational waves in semiclosed electromagnetic universes. Complete system of Newman-Penrose equations and radial dependence of the field variables. Soviet Physics Journal 30, 1023–1026 (1987). https://doi.org/10.1007/BF00897913

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  • DOI: https://doi.org/10.1007/BF00897913

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