A New Cosmological Model of Quintessence and Dark Matter
Astrophysics
2009-10-31 v3 High Energy Physics - Phenomenology
Abstract
We propose a new class of quintessence models in which late times oscillations of a scalar field give rise to an effective equation of state which can be negative and hence drive the observed acceleration of the universe. Our ansatz provides a unified picture of quintessence and a new form of dark matter we call "Frustrated Cold Dark Matter" (FCDM). FCDM inhibits gravitational clustering on small scales and could provide a natural resolution to the core density problem for disc galaxy halos. Since the quintessence field rolls towards a small value, constraints on slow-roll quintessence models are safely circumvented in our model.
Cite
@article{arxiv.astro-ph/9910097,
title = {A New Cosmological Model of Quintessence and Dark Matter},
author = {Varun Sahni and Limin Wang},
journal= {arXiv preprint arXiv:astro-ph/9910097},
year = {2009}
}
Comments
Revised. Important new results added in response to referees comments