Olga Avsajanishvili Reconstruction And Analysis Of Cosmological Scalar Field %cf%95cdm Models

Pdf Reconstruction Analysis And Constraints Of Cosmological Scalar Using mcmc analysis, the constraints of these models were obtained by comparing observations for the expansion rate of the universe, the angular diameter distance and the growth rate function. We studied the following scalar field ϕcdm models: ten quintessence models and seven phantom models. we reconstructed these models using the phenomenological method developed by our.

Pdf Cosmological Constrains On Minimally And Non Minimally Coupled We present cosmological parameter results from the final full mission planck measurements of the cosmic microwave background (cmb) anisotropies, combining information from the temperature and. Using the bayesian statistical analysis, we could not uniquely identify the preferable φcdm models compared to the fiducial Λcdm model based on the predicted desi data, and the Λcdm model is a true model. Abstract cosmological models that go beyond the standard lambda cold dark matter (Λcdm) scenario, namely, scalar field $phi$cdm models, are considered. Abstract: we studied the following scalar field φcdm models: ten quintessence models and seven phantom models. we reconstructed these models using the phenomenological method developed by our group.

Pdf Extended Analysis For The Evolution Of The Cosmological History Abstract cosmological models that go beyond the standard lambda cold dark matter (Λcdm) scenario, namely, scalar field $phi$cdm models, are considered. Abstract: we studied the following scalar field φcdm models: ten quintessence models and seven phantom models. we reconstructed these models using the phenomenological method developed by our group. Olga avsajanishvili | cosmological scalar field ϕcdm models cosmology from home 1.56k subscribers subscribed. Cosmological models of dark energy: theory and observations # 6 olga avsajanishvili ( ilia state u. ) (sep 1, 2019). Search across a wide variety of disciplines and sources: articles, theses, books, abstracts and court opinions. We investigated how well the chevallier polarsky linder (cpl) parametrization approximates the various scalar field models. we determined the location of scalar field model in the phase space of the cpl parameters.