Physics of Particles and Nuclei

, Volume 49, Issue 4, pp 514–519 | Cite as

Third Quantization and Emergence of the Quasiclassical Wave Function of the Universe

  • P. IvanovEmail author
  • S. V. Chernov


Quantized solutions of the Wheeler–DeWitt (WDW) equation describing a closed Friedmann–Robertson–Walker universe with a \(\Lambda \) term and a set of massless scalar fields are studied. It is shown that when \(\Lambda \ll 1\) units and the standard in-vacuum state is considered, the wave function of the universe \(\Psi \) behaves as a random quasiclassical field at rather large a, namely, \(1 \ll a \ll {{e}^{{\frac{2}{{3\Lambda }}}}}\) [1].



The work was supported by Grant NSh-6595.2016.2 of the President of the Russian Federation for Support of Leading Scientific Schools.


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Copyright information

© Pleiades Publishing, Ltd. 2018

Authors and Affiliations

  1. 1.Astro Space Centre, Lebedev Physical InstituteMoscowRussia

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