Quantum cosmological effects from the high redshift supernova observations

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dc.creatorKuzmichev, V. V.
dc.date2004-07-01
dc.date.accessioned2026-07-07T02:13:41Z
dc.date.available2026-07-07T02:13:41Z
dc.descriptionSubject of this contribution is to demonstrate that the observed faintness of the supernovae at the high redshift can be considered as a manifestation of quantum effects at cosmological scales. We show that observed redshift distribution of coordinate distances to the type Ia supernovae can be explained by the local manifestations of quantum fluctuations of the cosmological scale factor about its average value. These fluctuations can arise in the early universe, grow with time, and produce observed accelerating or decelerating expansions of space subdomains containing separate supernovae with high redshift whereas the universe as a whole expands at a steady rate.
dc.description22 pages, 7 EPS figures; a contribution to the International workshop on Frontiers of Particle Astrophysics, Kiev, June 21 - 24, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0407013
dc.identifierhttp://arxiv.org/abs/astro-ph/0407013
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7899
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectQuantum Physics
dc.titleQuantum cosmological effects from the high redshift supernova observations
dc.typetext

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