Colour entangled orphan quarks and dark energy from cosmic QCD phase transition

Details Colour entangled orphan quarks and dark energy from cosmic QCD phase transition Colour entangled orphan quarks and dark energy from cosmic QCD phase transition

2006-02-22

arxiv.org/abs/hep-ph/0602202v1

Nucl.Phys. A774 (2006) 769-774

Physics

High Energy Physics

High Energy Physics - Phenomenology

5 pages manuscript, To be published in proceedings of Quark Matter 2005

Scientific paper

10.1016/j.nuclphysa.2006.06.133

The present day astrophysical observations indicate that the universe is composed of a large amount of dark energy (DE) responsible for an accelerated expansion of the universe, along with a sizeable amount of cold dark matter (CDM), responsible for structure formation. The explanations for the origin or the nature of both CDM and DE seem to require ideas beyond the standard model of elementary particle interactions. Here we show that CDM and DE both can arise from the standard principles of strong interaction physics and quantum entanglement.

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