Cosmological distances scale. Part 15: cosmically jerk and the dipole of gravitational heterogeneity

Abstract

The central question of the cosmic shock in the series of articles “Cosmological Distance Scale” is considered: do the data for parametric identification of the Friedman-Robertson-Walker model in the form of a dependence of the photometric distance on the redshift of type Ia supernovae used in the work of the High-Z SN Search Team and Supernovae Cosmology Project allow us to consider the acceleration of the expansion of the Universe as the most plausible hypothesis on the criterion of the minimum error of inadequacy. The previously discovered discrepancies (changes in the structure and parameters of the systematic component of the model) and rank inversions of photometric distances of supernovae SN Ia for the systematic component of this model are analyzed. It is shown that the cause of these metric violations is the isotropy of the Friedman-Robertson-Walker model. In the anisotropic model of the cosmological distance scale, the disjunctions and rank inversions are associated with the orientation of the gravitational dipoles of the heterogeneity of the large-scale structure of the Universe. These dipoles represent diametrically opposite pairs of “super cluster galaxies – giant void” on the celestial sphere. Due to the size of only the super-void in the constellation Eridanus, comparable to the size of the observable part of the Universe, a colossal imbalance of the gravitational action of a massive super cluster of galaxies is created. This leads to disturbances in the form of disorders and rank inversions in isotropic Friedman-Robertson-Walker type models.