Constraints on the dark energy equation of state from the separation of CMB peaks and the evolution of alpha

Details Constraints on the dark energy equation of state from the separation of CMB peaks and the evolution of alpha Constraints on the dark energy equation of state from the separation of CMB peaks and the evolution of alpha

2005-04-28

arxiv.org/abs/astro-ph/0504650v1

Phys.Rev.D71:123528,2005

Astronomy and Astrophysics

Astrophysics

17pages, 14figures

Scientific paper

10.1103/PhysRevD.71.123528

We introduce a simple parametrization of the dark energy equation of state, \omega, which is motivated from theory and recent experimental data. The theory is related to the tracker solution to alleviate the fine tuning problem. Recent experimental data indicates that the present value of \omega is close to -1. We analyze the evolution of \omega from the separation of CMB peaks and the time variation of the fine structure constant, \alpha. We find that -1.00 \leq \omega^{(0)} \leq -0.971_{-0.027}^{+0.017} and 1.76_{-0.42}^{+0.29} \times 10^{-4} \leq (d \omega / dz)_{z=0} \leq 0.041_{-0.037}^{+0.016} at 95% confidence level (CL).

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