Do Bound Structures Brake Cosmic Acceleration?

In this paper we investigate the impact of the coupling between a quintessence field and clustered matter on the average equation of state of the scalar field. We take the NFW profile to be characteristic of bound structures on galactic and cluster scales, and the isothermal distribution to hold for...

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Bibliographic Details
Published inarXiv.org
Main Authors Schrempp, Lily, Brown, Iain A
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 09.06.2010
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