Properties of an ideal self-gravitating fluid with a barotropic equation of state in the equilibrium configurations and its vortex physical fields have been studied within the framework of general theory of relativity. In this case, the gravitational field of the liquid always contains a vortex component. It has been shown that with a proper choice of the system parameters, the solution of the Einstein equations describes the space-time geometry with wormholes resulting from the action of the vortex field. The wormholes in this case have plane asymptotes.
Similar content being viewed by others
References
V. G. Krechet, Russ. Phys. J., 50, No. 10, 1021–1025 (2007).
V. G. Krechet and D. V. Sadovnikov, Grav. Cosmol., 13, No. 4, 269–272 (2007).
K. A. Bronnikov, V. G. Krechet, and J. P. S. Lemos, Phys. Rev. D, 87, No. 8, 084060 (2013).
V. A. Rubakov, Theor. Math. Phys., 188, No. 2, 337–342 (2016).
I. D. Novikov and A. A. Shatskii, Zh. Eksp. Teor. Fiz., 141, No. 5, 919–923 (2012).
K. A. Bronnikov and V. G. Krechet, Int. J. Mod. Phys. A, 31, Nos. 2–3, 1641022 (2016).
Author information
Authors and Affiliations
Corresponding author
Additional information
Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 6, pp. 130–138, June, 2020.
Rights and permissions
About this article
Cite this article
Krechet, V.G., Oshurko, V.B. & Baidin, A.E. On the Properties of Stationary Distributions of Gravitational Vortex Fields and Continuous Media. Russ Phys J 63, 1045–1054 (2020). https://doi.org/10.1007/s11182-020-02135-y
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s11182-020-02135-y