A parameterized equation of state for dark energy and Hubble Tension

We propose a parameterized equation of state for dark energy and perform observational tests with the Hubble parameter measurements, the Pantheon supernova sample, baryon acoustic oscillations, and DESI DR2 data. We obtain the best-fit values for the parameters as: $H_0=73.96\pm 0.16$, $\Omega_{\rm m}=0.2434\pm 0.0079$, and $\alpha=-0.00049\pm 0.00092$, demonstrating that the model exhibits a high degree of consistency with astronomical observations and provides a promising parameterized method for addressing the Hubble tension.