arXiv · 1706.04522
Observational constraints on tensor perturbations in cosmological models with dynamical dark energy
Abstract
We constrain the contribution of tensor-mode perturbations with free $n_t$ in the models with dynamical dark energy with the barotropic equation of state using Planck-2015 data on CMB anisotropy, polarization and lensing, BICEP2/Keck Array data on B-mode polarization, power spectrum of galaxies from WiggleZ and SN Ia data from the JLA compilation. We also investigate the uncertainties of reconstructed potential of the scalar field dark energy.
Explore related subjects
Keep this discovery
O. Sergijenko. 2017-06-14. Observational constraints on tensor perturbations in cosmological models with dynamical dark energy. https://doi.org/10.5506/aphyspolbsupp.10.411
Cite the original work for its findings. Save a collection to share your selection of sources.