When did vacuum energy of the Universe become cosmological constant?

dc.creatorBurdyuzha, V.
dc.date2007-12-29
dc.date.accessioned2026-07-07T08:51:52Z
dc.date.available2026-07-07T08:51:52Z
dc.descriptionA quark-gluon phase transition in the Universe is researched after which vacuum (dark) energy has hardened and become cosmological constant. Before this a vacuum component of the Universe was changing by jumps during phase transitions since vacuum condensates of quantum fields carried a negative contribution in its positive density energy. This quintessence period of the Universe life took place during the first parts of a second when our Universe was losing high symmetry. Using Zel'dovich's formula the modern value of vacuum energy is also calculated. It is shown that a quantum chromodynamical vacuum which is characterized by pseudogoldstone bosons existed definitely when temperature of the Universe was T~150 MeV. Therefore there is a large probability that dark energy is vacuum energy.
dc.description3 pages. submitted to Phys. Letters
dc.identifierhttps://arxiv.org/abs/0801.0047
dc.identifierhttp://arxiv.org/abs/0801.0047
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/145088
dc.subjectHigh Energy Physics - Phenomenology
dc.titleWhen did vacuum energy of the Universe become cosmological constant?
dc.typetext

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