The quintessence field as a perfect cosmic fluid of constant pressure
Wenzhong Liu, Jun Ouyang, Huanxiong Yang

TL;DR
This paper explores a quintessence scalar field model with constant pressure, acting as dynamic dark energy, and analyzes its effects on cosmic evolution and structure growth.
Contribution
It introduces a quintessence model with constant pressure that interpolates between different cosmic epochs and examines its unique perturbation and clustering properties.
Findings
Quintessence density contrasts decay monotonously on sub-horizon scales.
The model alleviates the coincidence problem.
Quintessence impacts early structure growth despite decay in clustering.
Abstract
We study the cosmology of a quintessence scalar field which is equivalent to a non-barotropic perfect fluid of constant pressure. The coincidence problem is alleviated by such a quintessence equation-of-state that interpolates between plateau of zero at large redshifts and plateau of minus one as the redshift approaches to zero. The quintessence field is neither a unified dark matter nor a mixture of cosmological constant and cold dark matter, because the quintessence density contrasts decay monotonously on sub-horizon scales and the squared sound speeds of quintessence perturbations do not vanish. What a role does the quintessence play is dynamic dark energy. Though the clustering of quintessence decays drastically, it could remarkably impact the growth rate of the density perturbations of non-relativistic matters at early stage.
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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Solar and Space Plasma Dynamics
