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- W4382068691 abstract "Abstract In the current paper, a dark energy (DE) model reconstructed from the well‐motivated deceleration parameter (DP) is analyzed. A flat FRW Universe filled with radiation, dark matter (DM), and dark energy fluids is considered. The free parameters are constrained using measurements from Supernovae, Hubble, Gamma Ray Bursts, Quasars, and Baryon acoustic Oscillations. The model under study is found to be very supported by observation with respect to ΛCDM since . Besides, a cosmographic analysis is performed showing that the reconstructed model behaves similarly as ΛCDM does. Finally, a diagnostic analysis is performed reporting that the studied model behaves quintessence type at a late time." @default.
- W4382068691 created "2023-06-27" @default.
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- W4382068691 date "2023-06-25" @default.
- W4382068691 modified "2023-10-14" @default.
- W4382068691 title "Observational Constraining Study of New Deceleration Parameters in FRW Universe" @default.
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- W4382068691 doi "https://doi.org/10.1002/prop.202300033" @default.
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