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QUINTESSENCE AND THE FIRST DOPPLER PEAK
2001
Modern Physics Letters A
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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, Ω_k, for any value of the ratio Ω_Λ/Ω_M, so that such a dependence is perfectly valid in the range suggested by supernova observations.
doi:10.1142/s0217732301005394
fatcat:s6f65jiwtnhadiaszq6aqvtsqa