Color-charged Quark Matter in Astrophysics?

dc.creatorQiu, Congxin
dc.creatorXu, Renxin
dc.date2006-08-13
dc.date.accessioned2026-07-07T09:37:51Z
dc.date.available2026-07-07T09:37:51Z
dc.descriptionColor confinement is only a supposition, which has not been proved in QCD yet. It is proposed here that macroscopic quark gluon plasma in astrophysics could hardly maintain colorless because of causality. The authors expected that the existence of chromatic strange quark stars as well as chromatic strangelets preserved from the QCD phase transition in the early universe could be unavoidable if their colorless correspondents do exist.
dc.description3 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0608272
dc.identifierhttp://arxiv.org/abs/astro-ph/0608272
dc.identifierChin.Phys.Lett. 23 (2006) 3205-3207
dc.identifierdoi:10.1088/0256-307X/23/12/023
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/160607
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleColor-charged Quark Matter in Astrophysics?
dc.typetext

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