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.
Screening of Newtonian potential and dark matter problem
Advances in Space Research ; 31 , 2 ; 489-494
2002-01-01
6 pages
Article (Journal)
Electronic Resource
English
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