📝 SummarXiv

Abstract

We introduce three-parameter extensions of the two-parameter minimal Akhtar-Hossain (mAH) parametrization, termed modified minimal AH (MmAH1,2), which provide greater flexibility in the dynamics of dark energy. These models are compared with $\Lambda$CDM, $w$CDM, mAH, CPL, and three-parameter CPL (CPL-$w_{\rm b}$) using a joint data set of the CMB compressed likelihood, DESI DR2, Pantheon$+$ supernovae, $H(z)$ measurements, and redshift-space distortions. While the common cosmological parameters remain stable across models, CPL and the MmAH1,2 yield modest improvements in fit, with $\Delta\chi^2\simeq -6$ to $-7$ and corresponding $\Delta{\rm AIC}\simeq -1$ to $-2$ relative to $\Lambda$CDM, suggesting a mild preference for dynamical dark energy. Statistical consistency with $\Lambda$CDM is quantified via the Mahalanobis distance in one, two, and three dimensional parameter subspaces. In 1D, the strongest deviation occurs for MmAH1 ($2.5\sigma$), followed by CPL ($2.3\sigma$). In 2D, CPL-$w_{\rm b}$ shows the highest discrepancy ($2.3\sigma$), while other models remain at the $1.7$-$2.1\sigma$ level. In 3D, CPL-$w_{\rm b}$ continues to exhibit the largest tension ($\sim2\sigma$), though this arises in the presence of very strong correlations, particularly between $w_{\rm a}$ and $w_{\rm b}$, whereas the MmAH extensions display slightly weaker but still non-negligible discrepancies ($1.4$-$1.8\sigma$). Overall, these results indicate consistent evidence for departures from $\Lambda$CDM.