Dark matter, dark energy and gravity
| dc.contributor.author | Robson, B A | |
| dc.date.accessioned | 2015-12-08T22:39:08Z | |
| dc.date.issued | 2015 | |
| dc.date.updated | 2015-12-08T10:14:12Z | |
| dc.description.abstract | 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 massless 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. | |
| dc.identifier.issn | 0218-3013 | |
| dc.identifier.uri | http://hdl.handle.net/1885/36115 | |
| dc.publisher | World Scientific Publishing Company | |
| dc.source | International Journal of Modern Physics E - Nuclear Physics | |
| dc.title | Dark matter, dark energy and gravity | |
| dc.type | Journal article | |
| local.bibliographicCitation.issue | 2 | |
| local.bibliographicCitation.lastpage | 10 | |
| local.bibliographicCitation.startpage | 1 | |
| local.contributor.affiliation | Robson, B A, College of Physical and Mathematical Sciences, ANU | |
| local.contributor.authoruid | Robson, B A, u4043271 | |
| local.description.embargo | 2037-12-31 | |
| local.description.notes | Imported from ARIES | |
| local.identifier.absfor | 020203 - Particle Physics | |
| local.identifier.absseo | 970102 - Expanding Knowledge in the Physical Sciences | |
| local.identifier.ariespublication | u4726473xPUB132 | |
| local.identifier.citationvolume | 24 | |
| local.identifier.doi | 10.1142/S0218301315500123 | |
| local.identifier.scopusID | 2-s2.0-84928433533 | |
| local.type.status | Published Version |
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