Multi-Messenger Cosmology: A Route to Accurate Inference of Dark Energy Beyond CPL Parametrization from XG Detectors

Understand

One of the central challenges in modern cosmology is understanding the nature of dark energy and its evolution throughout the history of the Universe.

• Dark energy is commonly modeled as a perfect fluid with a time-varying equation-of-state parameter, $w(z)$, often modeled under CPL parametrization using two parameters $w_0$ and $w_a$.
• In this study, we explore both parametric and non-parametric methods to reconstruct the dark energy Equation of State (EoS) using Gravitational Wave (GW) sources, with and without electromagnetic (EM) counterparts called bright sirens and dark sirens respectively.
• In the parametric approach, we extend the widely used $w_0$-$w_a$ model by introducing an additional term, $w_b$, to better capture the evolving dynamics of dark energy up to high redshift which is accessible from GW sources.