Reconstructing the cosmic expansion with a generalized q(z) parameterization: A decelerating Universe from late-time constraints

TL;DR

This paper introduces a new generalized parameterization of the deceleration parameter q(z) that includes an effective radiative component, allowing for a more flexible reconstruction of cosmic expansion history from late-time observational data.

Contribution

It extends previous q(z) models by regulating high-redshift behavior and incorporating an effective radiative component, providing a more comprehensive framework for cosmic expansion analysis.

Findings

The universe is currently accelerating with q_0 ≈ -0.25.

The transition redshift z_T ≈ 0.80 occurs earlier than in ΛCDM.

Data suggests a possible reduction in late-time acceleration.

Abstract

We present a generalized phenomenological parameterization of the deceleration parameter $q(z)$ that incorporates an effective radiative component (ERC) in addition to a localized late-time contribution. The proposed framework extends previous two-parameter $q(z)$ reconstructions by explicitly regulating the high-redshift behavior while preserving the late-time transition dynamics. We constrain the free parameters $(h, q_0, z_c, z_e)$ using late-time observational data from cosmic chronometers (CC), Pantheon+ Type Ia supernovae (SNIa), H\,\textsc{ii} galaxies (HIIG), and intermediate-luminosity quasars (QSO). For the full data combination (CC+SNIa+HIIG+QSO), we obtain $q_0 = -0.25^{+0.04}_{-0.04}$ and a transition redshift $z_T \simeq 0.80$, indicating a currently accelerating Universe with a transition occurring earlier than in the $\Lambda$CDM model. Within the redshift range probed by the data, the reconstructed $q(z)$ deviates from the $\Lambda$CDM trend, suggesting a possible reduction of the late-time acceleration. Furthermore, the reconstruction favors a relatively high value of the Hubble parameter, $h = 0.729 \pm 0.006$. The ERC remains weakly constrained by late-time data but ensures a smooth and monotonic evolution of $q(z)$, $j(z)$, and $w_{\rm eff}(z)$ across a wide redshift range. Within the observed interval, the model effectively reproduces the late-time behavior of the previous parametrization, while providing a controlled extension toward early epochs. Our results show that current low- and intermediate-redshift data are compatible with a reduced late-time acceleration.