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

Shibaji Banerjee; Abhijit Bhattacharyya; Sanjay K. Ghosh; Ernst-Michael lgenfritz; Sibaji Raha; Bikash Sinha; Eiichi Takasugi; Hiroshi Toki

doi:10.1016/j.nuclphysa.2006.06.133

arXiv · hep-ph/0602202

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

Shibaji Banerjee·Abhijit Bhattacharyya·Sanjay K. Ghosh·Ernst-Michael lgenfritz·Sibaji Raha·Bikash Sinha·Eiichi Takasugi·Hiroshi Toki

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Abstract

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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Shibaji Banerjee, Abhijit Bhattacharyya, Sanjay K. Ghosh, Ernst-Michael lgenfritz, Sibaji Raha, Bikash Sinha, Eiichi Takasugi, Hiroshi Toki. 2006-02-22. Colour entangled orphan quarks and dark energy from cosmic QCD phase transition. https://doi.org/10.1016/j.nuclphysa.2006.06.133

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