Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-12-06
Astrophys.J. 559 (2001) 501-506
Astronomy and Astrophysics
Astrophysics
Replaced with version to appear in Astrophysical Journal
Scientific paper
10.1086/322253
We propose that it should be possible to use the CMB to discriminate between dark energy models with different equations of state, including distinguishing a cosmological constant from many models of quintessence. The separation of peaks in the CMB anisotropies can be parametrised by three quantities: the amount of quintessence today, the amount at last scattering, and the averaged equation of state of quintessence. In particular, we show that the CMB peaks can be used to measure the amount of dark energy present before last scattering.
Doran Michael
Lilley Matthew
Schwindt Jan
Wetterich Christof
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