  It has been theorized that Dynamical Dark Energy (DDE) could be a possible
solution to the Hubble tension. To avoid the degeneracy between the Hubble
parameter $H_0$ and the sound horizon scale $r_d$, in this article we use their
multiplication as one parameter $c/\left(H_0 r_d\right)$ and we use it to infer
cosmological parameters for 6 different models - $\Lambda$CDM and 5 DDE
parametrizations -- the Chevallier-Polarski-Linder (CPL), the Barboza-Alcaniz
(BA), the Low correlation (LC), the Jassal-Bagla-Padmanabhan (JBP) and the
Feng-Shen-Li-Li model. We choose a dataset that treats this combination as one
parameter, that includes the Baryon Acoustic Oscillation (BAO) data $0.11 \le z
\le 2.40$ and additional points from the Cosmic Microwave Background (CMB)
Peaks ($z \approx 1090$). To them, we add the marginalized Pantehon dataset and
GRB dataset. We see that the tension is moved from $H_0$ and $r_d$ to
$c/\left(H_0 r_d\right)$ and $\Omega_m$. There is only one model that satisfies
the Planck 2018 constraints on both parameters and this is LC with a huge
error. The rest cannot fit into both constraints. $\Lambda$CDM is preferred
with respect to the statistical measures.
