Observables and unobservables in dark energy cosmologies
@article{Amendola2013ObservablesAU, title={Observables and unobservables in dark energy cosmologies}, author={L. Amendola and M. Kunz and M. Motta and I. D. Saltas and I. Sawicki}, journal={Physical Review D}, year={2013}, volume={87}, pages={023501} }
The aim of this paper is to answer the following two questions: (1) Given cosmological observations of the expansion history and linear perturbations in a range of redshifts and scales as precise as is required, which of the properties of dark energy could actually be reconstructed without imposing any parameterization? (2) Are these observables sufficient to rule out not just a particular dark energy model, but the entire general class of viable models comprising a single scalar field?
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