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Bouncing Universe and Reconstructing Vector Field

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arxiv 1001.4682 v1 pith:C5F4WXUP submitted 2010-01-26 hep-th

J. Sadeghi , M. R. Setare , A. R. Amani , S. M. Noorbakhsh This is my paper · ORCID
classification hep-th
keywords vectorfieldbouncingconsidercoupledmassivemodelnon-minimally
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Motivated by the recent works of Refs. \cite{R1, R2} where a model of inflation has been suggested with non-minimally coupled massive vector fields, we generalize their work to the study of the bouncing solution. So we consider a massive vector field, which is non-minimally coupled to gravity. Also we consider non-minimal coupling of vector field to the scalar curvature. Then we reconstruct this model in the light of three forms of parametrization for dynamical dark energy. Finally we simply plot reconstructed physical quantities in flat universe.

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  1. Observational analysis of bulk viscous modified Chaplygin gas in (2+1)-dimensional universe using MCMC

    gr-qc 2025-04 reject novelty 4.0 of 10

    A (2+1)-dimensional bulk viscous Chaplygin gas model is fit to H(z) and Pantheon data via MCMC, but the derivation and the reported Planck-consistent H0 rest on inconsistent equations and hidden assumptions.

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