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A Star of Vacuum-like Matter

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Abstract

A model of a star consisting of vacuum-like matter is constructed in the framework of general relativity. Its stability and other physical properties are analyzed. This stellar model is compared with cosmological models consisting of the same vacuum-likematter with a pressure equal to the energy density but with the opposite sign.

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Author information

Authors and Affiliations

  1. Astro Space Center, P.N. Lebedev Physical Institute, Russian Academy of Sciences, Moscow, 117997, Russia

    I. D. Novikov & D. I. Novikov

  2. Niels Bohr International Academy, Niels Bohr Institute, Copenhagen, Denmark

    I. D. Novikov

  3. National Research Center Kurchatov Institute, Moscow, 123182, Russia

    I. D. Novikov

Authors
  1. I. D. Novikov
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  2. D. I. Novikov
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Corresponding author

Correspondence to I. D. Novikov.

Additional information

Russian Text © I.D. Novikov, D.I. Novikov, 2019, published in Astronomicheskii Zhurnal, 2019, Vol. 96, No. 4, pp. 284–287.

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Novikov, I.D., Novikov, D.I. A Star of Vacuum-like Matter. Astron. Rep. 63, 289–292 (2019). https://doi.org/10.1134/S106377291904005X

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  • DOI: https://doi.org/10.1134/S106377291904005X

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