Quintessence and the first Doppler peak
Astrophysics
2009-11-06 v1
Abstract
By using a tracking quintessence model we obtain that the position of the first Doppler peak in the spectrum of CMB anisotropies only depends on the topology of the universe, , for any value of the ratio , so that such a dependence is perfectly valid in the range suggested by supernova observations.
Cite
@article{arxiv.astro-ph/0103194,
title = {Quintessence and the first Doppler peak},
author = {Pedro F. Gonzalez-Diaz},
journal= {arXiv preprint arXiv:astro-ph/0103194},
year = {2009}
}
Comments
9 pages, LaTex