Cosmological Dynamics of Exponential Quintessence Constrained by BAO, Cosmic Chronometers, and DES-SN5YR/Pantheon+ Data
Sanjeeda Sultana, Surajit Chattopadhyay

TL;DR
This paper tests an exponential quintessence cosmological model against recent observational data, finding it consistent with observations and comparable to LCDM, with detailed parameter constraints and physical viability analysis.
Contribution
It provides the first comprehensive observational constraints on an exponential quintessence model using multiple high-precision datasets, demonstrating its viability and similarity to LCDM.
Findings
Model parameters are tightly constrained by data.
The model predicts H(z) and mu(z) consistent with observations.
Energy conditions and diagnostics support physical viability.
Abstract
We perform a comprehensive observational test of a canonical quintessence model driven by an exponential potential, motivated by its emergence in higher-dimensional theories, string-inspired scenarios, and modified gravity. Using a Markov Chain Monte Carlo framework, we constrain the model with the latest high-precision observational datasets including Cosmic Chronometers, Baryon Acoustic Oscillation, Pantheon+, and DES-SN5YR Type Ia Supernovae. The combined data significantly tighten the parameter bounds on (H0, Omega_m0, eta0, gamma) and yield predictions for the Hubble parameter H(z), the distance modulus mu(z), and the scaled comoving angular diameter distance that remain in excellent agreement with observations and closely follow the LCDM baseline. An information-theoretic model comparison using the Akaike Information Criterion shows that the exponential quintessence model remains…
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