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This study examines cosmological parameters beyond the standard Lambda-CDM model using the latest cosmic microwave background data, DESI baryon acoustic oscillations measurements, and supernovae catalogs. The analysis systematically tests extensions involving dark energy dynamics, spatial curvature, neutrino properties, and inflationary parameters. The researchers find consistent evidence for dynamical dark energy across all extended models tested, while other deviations from the standard model remain largely insignificant, and notably, none of the extensions resolve the Hubble constant tension.
Why it matters
These findings help constrain fundamental properties of the universe and guide future cosmological research priorities. The persistent preference for dynamical dark energy over a cosmological constant, combined with the failure to resolve key tensions like the Hubble constant discrepancy, suggests either new physics or systematic issues requiring further investigation.
Understand the Science
arXiv:2607.01226v1 Announce Type: new
Abstract: We present a systematic reassessment of cosmological constraints beyond $Lambda$CDM by progressively relaxing the assumptions underlying Dark Energy (DE), Curvature, Neutrinos, and Inflation. Using the latest CMB data together with DESI BAO and different SN catalogues, we show that the preference for dynamical DE persists across all the extended cosmologies considered. $Omega_k$ remains compatible with flatness, despite a mild $2.2sigma$ preference for $Omega_k>0$ that is substantially degraded in dynamical DE extensions. Constraints on $N_{rm eff}$ are broadly consistent with $N_{rm eff}=3.04$, while cosmological upper limits on the total neutrino mass vary substantially across the cosmologies explored, ranging from $sum m_nulesssim 0.06$ eV to $lesssim 0.2$ eV. We quantify both the preference for the mass ordering and the apparent tension between cosmology and oscillation experiments, showing that they are strongly framework dependent. We find no evidence for inflationary tensor modes, with $rlesssim 0.035$. Constraints on the spectral index $n_s$ show significant model dependence. Allowing for the scalar runnings produces a mild shift toward $alpha_s>0$ and $beta_s>0$ that can reabsorb the preference for larger $n_s$ found in small-scale CMB data, although both $alpha_s$ and $beta_s$ remain consistent with zero at $sim 1.5sigma$. We highlight the implications for slow-roll inflation and benchmark models. None of the extensions considered here can resolve the $H_0$ tension. We discuss the implications for $Omega_m$ and $S_8$. Overall, dynamical DE is the only significant deviation from $Lambda$CDM and has the strongest impact on the inferred conclusions in the other sectors of the model.
Source: Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation