2000/05/31 by Vinod B. Johri, V. B. Johri · 3 citations
Physics and Astronomy · #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Galaxies: Formation, Evolution, Phenomena #astro-ph #gr-qc #hep-ph
paper · pdf · doi:10.1103/physrevd.63.103504
published as Phys.Rev. D63 (2001) 103504 · 8 pages, Latex file, 1 figure, comments added
openalex publication_date 2001/04/12 · arxiv created 2001/05/06 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The role of the quintessence field as a probable candidate for the repulsive dark energy, the conditions for tracking and the requisites for tracker fields are examined. The concept of ``integrated tracking'' is introduced and a new criterion for the existence of tracker potentials is derived assuming monotonic increase in the scalar energy density parameter \ensuremathΩ_\ensuremathφ with the evolution of the universe as suggested by the astrophysical constraints. It provides a technique to investigate generic potentials of the tracker fields. The general properties of the tracker fields are discussed and their behavior with respect to the tracking parameter \ensuremathε is analyzed. It is shown that the tracker fields around the limiting value \ensuremathε\ensuremath≃(2)/(3) give the best fit with the observational constraints.