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 |
Files in This Item:
File | Description | Size | Format | |
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burgazli.pdf | 278.41 kB | Adobe PDF | View/Open |
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