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Scalar field potentials for cosmology

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 09 Apr 2004Embargo end date: 01 Jan 2004 English Publisher:American Physical Society (APS)Journal:Physical Review D, volume 69 (issn: 1550-7998, eissn: 1550-2368, Copyright policy )
Authors: Cardenas, VH; del Campo, S;

doi: 10.1103/physrevd.69.083508 , 10.48550/arxiv.astro-ph/0401031

arXiv: astro-ph/0401031

handle: 10533/175450

Scalar field potentials for cosmology

Abstract

We discuss different aspects of modern cosmology through a scalar field potential construction method. We discuss the case of negative potential cosmologies and its relation with oscillatory cosmic evolution, models with a explicit interaction between dark energy and dark matter which address the coincidence problem and also the case of non-zero curvature space.

5 pages, 2 figures, to be published in PRD

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Keywords

Astrophysics (astro-ph), FOS: Physical sciences, 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!
9
Average
Average
Average
Green
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