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Paper The following article is Open access

Gravitationally neutral dark matter–dark antimatter universe crystal with epochs of decelerated and accelerated expansion

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Published under licence by IOP Publishing Ltd
, , Citation I A Gribov and S A Trigger 2016 J. Phys.: Conf. Ser. 774 012045 DOI 10.1088/1742-6596/774/1/012045

1742-6596/774/1/012045

Abstract

A large-scale self-similar crystallized phase of finite gravitationally neutral universe (GNU)—huge GNU-ball—with spherical 2D-boundary immersed into an endless empty 3D- space is considered. The main principal assumptions of this universe model are: (1) existence of stable elementary particles-antiparticles with the opposite gravitational "charges" (M+gr and M-gr), which have the same positive inertial mass Min = |M±gr| ≥ 0 and are equally presented in the universe during all universe evolution epochs; (2) the gravitational interaction between the masses of the opposite charges" is repulsive; (3) the unbroken baryon-antibaryon symmetry; (4) M+gr-M-gr "charges" symmetry, valid for two equally presented matter-antimatter GNU-components: (a) ordinary matter (OM)-ordinary antimatter (OAM), (b) dark matter (DM)-dark antimatter (DAM). The GNU-ball is weightless crystallized dust of equally presented, mutually repulsive (OM+DM) clusters and (OAM+DAM) anticlusters. Newtonian GNU-hydrodynamics gives the observable spatial flatness and ideal Hubble flow. The GNU in the obtained large-scale self-similar crystallized phase preserves absence of the cluster-anticluster collisions and simultaneously explains the observable large-scale universe phenomena: (1) the absence of the matter-antimatter clusters annihilation, (2) the self-similar Hubble flow stability and homogeneity, (3) flatness, (4) bubble and cosmic-net structures as 3D-2D-1D decrystallization phases with decelerative (a ≤ 0) and accelerative (a ≥ 0) expansion epochs, (5) the dark energy (DE) phenomena with ΛVACUUM = 0, (6) the DE and DM fine-tuning nature and predicts (7) evaporation into isolated huge M±gr superclusters without Big Rip.

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10.1088/1742-6596/774/1/012045