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Probing decisive answers to dark energy questions from cosmic complementarity and lensing tomography
cosmic complementarity and lensing tomography
cosmic complementarity and lensing tomography
2.2 Dark energy parameterization As mentioned earlier, constraining the dark energy using its equation of state is known to be parameterization dependent, e.g. (Wang & Tegmark (2004); Upadhye et al. (2004)), and also suffers from a smearing due to the double integration involved (Maor et al. (2002); Maor et al. (2001)). Alternatively, one can probe directly the variations of the dark energy density as a function of redshift ρde(z). On the other hand, it has been argued that the equation of ...
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