2017
DOI: 10.5506/aphyspolbsupp.10.411
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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.PACS numbers: 95.36.+x, 98.80.-k

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“…The models with parameters on upper 1σ and 2σ confidence limits are quintessential, those with parameters on lower 1σ and 2σ confidence limits are phantom. This is in agreement with results obtained in [20] for the cosmological model with free tensor spectral index n t .…”
Section: Resultssupporting
confidence: 92%
“…The models with parameters on upper 1σ and 2σ confidence limits are quintessential, those with parameters on lower 1σ and 2σ confidence limits are phantom. This is in agreement with results obtained in [20] for the cosmological model with free tensor spectral index n t .…”
Section: Resultssupporting
confidence: 92%