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Dark matter, dark energy and gravity

dc.contributor.authorRobson, B A
dc.date.accessioned2015-12-08T22:39:08Z
dc.date.issued2015
dc.date.updated2015-12-08T10:14:12Z
dc.description.abstractWithin 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.issn0218-3013
dc.identifier.urihttp://hdl.handle.net/1885/36115
dc.publisherWorld Scientific Publishing Company
dc.sourceInternational Journal of Modern Physics E - Nuclear Physics
dc.titleDark matter, dark energy and gravity
dc.typeJournal article
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage10
local.bibliographicCitation.startpage1
local.contributor.affiliationRobson, B A, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidRobson, B A, u4043271
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020203 - Particle Physics
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationu4726473xPUB132
local.identifier.citationvolume24
local.identifier.doi10.1142/S0218301315500123
local.identifier.scopusID2-s2.0-84928433533
local.type.statusPublished Version

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