No, it does not prove. Several authors have shown possible ways for the warp drive not to violate the energy conditions in specific cases [1,2,3]. Santiago et al. assumed those authors claimed the energy conditions are always respected but merely asserted are not always violated. These results [1,2,3] are counter-proof to theorems that assume generic warp drives always violate energy conditions, which does not invalidate the contributions of authors who tried to prove such theorems. Much of this discussion comes from Alcubierre's (1994) claim [4] that for his warp drive metric
$$ ds^2 = - d t^2 + (d x + \beta d t)^2 + d y^2 + d z^2\,, $$
for the Eulerian observers with 4-velocities given by
$$ u_\mu = (-1,0,0,0) \ \ , \ \ u^\mu = (1,-\beta,0,0) \,, $$
the energy density, as measured by those observers, can be obtained as
$$ G^{\mu\nu} u_\mu u_\nu = -\frac{1}{4} \left[\left( \frac{\partial \beta}{\partial y} \right)^2 + \left( \frac{\partial \beta}{\partial z} \right)^2 \right] \leq 0\,
\label{negeng} $$
and the above expression equals $G^{00}$, so Alcubierre concluded considering Einstein equations $G^{\mu\nu} = T^{\mu\nu}$ that the term $T^{00}$ regarded as the energy density for the energy-momentum tensor is always negative, and that the warp drive always violates the weak (WEC) and dominant (DEC) energy conditions. Alcubierre's claim is not wrong. However, he did not account for vacuum and complex solutions for Einstein's equations. If the shift vector is found to be of complex value, it is possible that the complex part will be negative and the real part will be positive. So, the WEC and DEC are not always violated. The validity conditions for theorems that state that any warp drive class always violates the energy conditions must be reviewed.
PS: The energy conditions are not general theorems. They are axioms used by Hawking and others to prove the "no-hair theorem for black holes". Several experimental pieces of evidence violate those conditions, i.e., cosmic inflation, negative energy density in cavities (Casimir effect), dark energy, etc.
References
[1] https://arxiv.org/abs/2102.06824
[2] https://arxiv.org/abs/2006.07125
[3] https://arxiv.org/abs/2104.06488
[4] https://arxiv.org/abs/gr-qc/0009013
[5] https://link.springer.com/article/10.1140/epjc/s10052-021-09484-z