$\mathbf{\Omega_1\Omega_2}$-$\mathbf{\Lambda}$CDM: A promising phenomenological extension of the standard model of cosmology
Suresh Kumar

TL;DR
This paper introduces an extended cosmological model, $oldsymbol{\Omega_1oldsymbol{\Omega_2}}$-$oldsymbol{\Lambda}$CDM, adding terms to dark energy density, which fits observational data well and offers a flexible late-time universe evolution.
Contribution
It proposes a novel phenomenological extension to $oldsymbol{\Lambda}$CDM$, incorporating additional terms in the energy density expansion, and demonstrates its consistency with observational data.
Findings
The model fits Planck and DESI data effectively.
It predicts a Hubble constant consistent with TRGB measurements.
Dark energy equation of state shows a smooth transition across the phantom divide.
Abstract
We investigate a phenomenological extension of the standard CDM framework, the -CDM model, in which the total energy density of the universe is expanded in powers of . This parameterization recovers CDM and introduces two additional terms, and , in the dark energy sector alongside the cosmological constant, leading to a physically interpretable and observationally testable effective dark energy dynamics. Using Planck cosmic microwave background (CMB) data, we find that the model allows additional freedom in the late-time expansion history while preserving standard early-universe physics. When DESI baryon acoustic oscillation (BAO) data are included, the inferred Hubble constant is (68% CL), consistent with Tip of the Red Giant Branch (TRGB) measurements…
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Taxonomy
TopicsCosmology and Gravitation Theories · Particle physics theoretical and experimental studies · Galaxies: Formation, Evolution, Phenomena
