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Viscous dark fluid

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Mar 2008Embargo end date: 01 Jan 2007 English Publisher:Elsevier BVJournal:Physics Letters B, volume 661, pages 75-77 (issn: 0370-2693, Copyright policy )
Authors: Folomeev, Vladimir; Gurovich, Victor;

doi: 10.1016/j.physletb.2008.01.068 , 10.48550/arxiv.0710.0210

arXiv: 0710.0210

Viscous dark fluid

Abstract

The unified dark energy and dark matter model within the framework of a model of a continuous medium with bulk viscosity (dark fluid) is considered. It is supposed that the bulk viscosity coefficient is an arbitrary function of the Hubble parameter. The choice of this function is carried out under the requirement to satisfy the observational data from recombination ($z\approx 1000$) till present time.

4 pages, 1 figure, added references

Related Organizations
Keywords

Nuclear and High Energy Physics, Dark energy, Astrophysics (astro-ph), Dark matter, FOS: Physical sciences, Viscous fluid, Astrophysics

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    popularity
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    influence
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
14
Average
Average
Top 10%
Green
gold