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A tracker solution to the cold dark matter cosmic coincidence problem

1999/06/29 by Ivaylo Zlatev, Paul J. Steinhardt · 1 citation
Physics and Astronomy · #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Galaxies: Formation, Evolution, Phenomena #astro-ph #hep-ph

paper · pdf · doi:10.1016/s0370-2693(99)00707-8

published as Phys.Lett.B459:570-574,1999 · 8 pages, 2 eps figures, use epsfig.sty, accepted for publication in Physics Letters B

arxiv created 1999/06/29 · openalex publication_date 1999/07/01 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

Recently, we introduced the notion of "tracker fields," a form of quintessence which has an attractor-like solution. Using this concept, we showed how to construct models in which the ratio of quintessence to matter densities today is independent of initial conditions. Here we apply the same idea to the standard cold dark matter component in cases where it is composed of oscillating fields. Combining these ideas, we can construct a model in which quintessence, cold dark matter, and ordinary matter all contribute comparable amounts to the total energy density today irrespective of initial conditions.

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