Quintessence and the first Doppler peak

Details Quintessence and the first Doppler peak Quintessence and the first Doppler peak

2001-03-13

arxiv.org/abs/astro-ph/0103194v1

Mod.Phys.Lett. A16 (2001) 2003-2012

Astronomy and Astrophysics

Astrophysics

9 pages, LaTex

Scientific paper

10.1142/S0217732301005394

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, $\Omega_k$, for any value of the ratio
$\Omega_{\Lambda}/\Omega_M$, so that such a dependence is perfectly valid in
the range suggested by supernova observations.

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