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Cosmological Parameters from the Thermodynamic Model of Gravity

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Abstract

Within our recent thermodynamic model of gravity the dark energy is identified with the energy of collective gravitational interactions of all particles in the universe, which is missing in the standard treatments. For a simple model universe composed of neutral and charged particles of identical mass we estimate the radiation, baryon and dark energy densities and obtain the values which are very close to the current cosmological observations.

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Authors and Affiliations

  1. Andronikashvili Institute of Physics, 6 Tamarashvili Street, 0177, Tbilisi, Georgia

    Merab Gogberashvili

  2. Javakhishvili State University, 3 Chavchavadze Avenue, 0128, Tbilisi, Georgia

    Merab Gogberashvili

  3. National Quantum Information Center of Gdańsk, ul. Wł. Andersa 27, 81-824, Sopot, Poland

    Igor Kanatchikov

Authors
  1. Merab Gogberashvili
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  2. Igor Kanatchikov
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Correspondence to Merab Gogberashvili.

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Gogberashvili, M., Kanatchikov, I. Cosmological Parameters from the Thermodynamic Model of Gravity. Int J Theor Phys 53, 1779–1783 (2014). https://doi.org/10.1007/s10773-013-1976-6

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  • DOI: https://doi.org/10.1007/s10773-013-1976-6

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