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Rotating quantum cosmological models with wave fields

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

Abstract

The quantum evolution of homogeneous rotating cosmological models of the Gödel type with spinor and scalar fields is considered within the framework of the formalism of superspace quantization. De Witt's equation for a rotating cosmological model is shown to take the form of a Schrödinger equation in which the role of time is played by the phase of the spinor field, and it becomes possible to determine correctly the probability that rotating models lacking an initial singularity exist.

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Literature cited

  1. V. G. Krechet, Izv. Vyssh. Uchebn. Zaved., Fiz., No. 12, 9 (1985).

  2. T. Cristodoulakis and J. Zanelli, Preprint IC (227), Trieste (1983).

  3. V. G. Krechet, Izv. Vyssh. Uchebn. Zaved., Fiz., No. 3, 15 (1990).

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Authors
  1. V. G. Krechet
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Additional information

K. D. Ushinskii Yaroslav Pedagogical Institute. Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 1, pp. 41–44, January, 1993.

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Krechet, V.G. Rotating quantum cosmological models with wave fields. Russ Phys J 36, 33–35 (1993). https://doi.org/10.1007/BF00559252

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  • DOI: https://doi.org/10.1007/BF00559252

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