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Dynamic Cosmological Tests

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Astrophysics Aims and scope

A new class of cosmological tests is proposed which examines the dependence on redshift z of the dispersion in peculiar velocities, virial mass, and mass-luminosity ratios of galactic clusters. Data on galactic clusters with redshifts up to z ≈ 2 are accessible to modern instruments in the visible and x-ray ranges. Clusters of galaxies are less susceptible to evolutionary effects than other objects at large z, so that the proposed tests offer promise for analysis of cosmological models.

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Author information

Authors and Affiliations

  1. St. Petersburg Branch of the Special Astrophysical Observatory of the Russian Academy of Sciences, St. Petersburg, Russia

    A. A. Raikov

  2. Main (Pulkovo) Astronomical Observatory, Russian Academy of Sciences, St. Petersburg, Russia

    A. A. Raikov & E. A. Popova

  3. St. Petersburg State University, St. Petersburg, Russia

    V. V. Orlov

Authors
  1. A. A. Raikov
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  2. E. A. Popova
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  3. V. V. Orlov
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Corresponding author

Correspondence to A. A. Raikov.

Additional information

V. V. Orlov is deceased

Translated from Astrofizika, Vol. 61, No. 4, pp. 615-622 (November 2018).

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Raikov, A.A., Popova, E.A. & Orlov, V.V. Dynamic Cosmological Tests. Astrophysics 61, 539–545 (2018). https://doi.org/10.1007/s10511-018-9556-3

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  • DOI: https://doi.org/10.1007/s10511-018-9556-3

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