Dark matter, dark energy and gravity

被引：1

作者：

Robson, B. A. ^{[1
]}

机构：

[1] Australian Natl Univ, Res Sch Phys & Engn, Dept Theoret Phys, Acton, ACT 2601, Australia

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS E-NUCLEAR PHYSICS | 2015年 / 24卷 / 02期

关键词：

Dark matter; dark energy; gravity; generation model; NEWTONIAN DYNAMICS; COSMOLOGICAL CONSTANT; MASS; GALAXIES; HYPOTHESIS; SUPERNOVAE; UNIVERSE; MODEL;

D O I：

10.1142/S0218301315500123

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

Within the framework of the Generation Model (GM) of particle physics, gravity is identified with the very weak, universal and attractive residual color interactions acting between the colorless particles of ordinary matter (electrons, neutrons and protons), which are composite structures. This gravitational interaction is mediated by mass-less vector bosons (hypergluons), which self-interact so that the interaction has two additional features not present in Newtonian gravitation: (i) asymptotic freedom and (ii) color confinement. These two additional properties of the gravitational interaction negate the need for the notions of both dark matter and dark energy.

引用

页数：10

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