Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/4735
Title: QUINTESSENCE AND PHANTOM ENERGY INHOMOGENEITIES AT LATE STAGES OF UNIVERSE EVOLUTION
Authors: Burgazli, A. Yu.
Eingorn, Maxim V.
Zhuk, Oleksandr I.
Citation: Odessa Astronomical Publications
Issue Date: 2012
Publisher: Astroprint
Keywords: quintessence
phantom field
scalar perturbation
cosmology
Series/Report no.: ;vol. 25, issue 2, p. 125.
Abstract: ABSTRACT. As it directly follows from the scalar perturbations, applied to the late stages of evolution of the Universe, filled with dark energy, nonrelativistic matter and, possibly, quintessence or phantom energy, the last two components can not be homogeneous. We demonstrate that ω=-1/3 is only admissible negative parameter in the non-vacuum equation of state, determine the corresponding gravitational potentials and discuss their main properties.
Description: Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2012 . – Vol.25/2.
URI: http://dspace.onu.edu.ua:8080/handle/123456789/4735
Appears in Collections:Odessa Astronomical Publications

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