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Outer parts of large galactic clusters in the presence of dark energy

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Abstract

Dark energy limits a radius of big clusters of galaxies, and may accelerate hot gas outflowing from the cluster as a wind. Collision of accelerated winds, in presence of a magnetic field, produce a situation favorable for acceleration of EHECR.

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Authors and Affiliations

  1. Space Research Institute, Russian Academy of Sciences, Moscow, Russia

    G. S. Bisnovatyi-Kogan

  2. National Research Nuclear University MEPhI, Moscow, Russia

    G. S. Bisnovatyi-Kogan

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  1. G. S. Bisnovatyi-Kogan
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Correspondence to G. S. Bisnovatyi-Kogan.

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Bisnovatyi-Kogan, G.S. Outer parts of large galactic clusters in the presence of dark energy. Astron. Rep. 59, 430–440 (2015). https://doi.org/10.1134/S1063772915060049

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  • DOI: https://doi.org/10.1134/S1063772915060049

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