  The recent result from the DESI (Dark Energy Spectroscopic Instrument) data
release 1 (DR1) combined with the cosmic microwave background and supernova
data shows a preference for the dynamical dark energy over the cosmological
constant [1]. For this analysis, the Chevallier-Polarski-Linder (CPL)
parameterization of the dark energy equation of state has been used. Though CPL
parametrization is the most popular parametrization of dark energy equation of
state (EoS) recent studies have questioned its choice of prior and degeneracy.
In this work, we propose a new parametrization of the dark energy equation of
state motivated by its ability to cross the phantom barrier crossing. At a high
redshift limit, this parametrization takes the form of CPL parametrization. We
have used the Bayesian model selection criteria in which this parametrisation
shows a moderate positive preference over the $\Lambda$CDM model. Contrary to
the DESI2024 results our model suggests the current value of the dark energy
equation of state to be phantom today with two phantom barrier crossings one at
$z\simeq 0.4$ from deep phantom to quintessence which matches with the finding
from the DESI2024 result and another phantom barrier crossing very recently at
$z\simeq0.1$ from quintessence to phantom. The proposed model also weakens the
Hubble tension significantly to $\approx 2 \sigma$ while comparing with the
result from [2] and to $\approx 1.4 \sigma$ while comparing with [3].
