AbstractThe long-range periodicity of the Universe is well recognized now and the characteristic wave number of the pair correlation function (PCF) k0 ∼ 0.05 h Mpc−1 (λ0 ∼ 125 h−1 Mpc) is well-defined. Here we point to the fact that along with the long-wave oscillations the observable data presented by da Costa et al. (1994), Einasto et al. (1997b) and Einasto et al. (1998) are indicative of short-wave oscillations of k ∼ 0.2 ÷ 0.4 h Mpc−1 (λ ∼ 20 ÷ 40 h−1 Mpc). We propose also an interpretation of the observed oscillating behaviour of PCF based on our theory of dynamical screening of the gravitational potential.


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    Title :

    Screening of Newtonian potential and dark matter problem


    Contributors:

    Published in:

    Advances in Space Research ; 31 , 2 ; 489-494


    Publication date :

    2002-01-01


    Size :

    6 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



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