  In this work, we investigate the dynamics of bouncing cosmologies within the
framework of Weyl-type $f(Q,T)$ gravity. Here, $Q$ represents the non-metricity
of the space-time, is determined by the vector field $w_\mu$, while $T$
represents the trace of the matter energy-momentum tensor. Our objective is to
explore the feasibility of avoiding the Big Bang singularity by implementing a
matter-bounce cosmology. To achieve this, we consider a specific model with the
functional form $f(Q,T)=\alpha Q+\frac{\beta }{6\kappa ^2}T$, where $\alpha$
and $\beta$ are model parameters. We analyze the dynamical parameters
associated with this model and examine the influence of the Weyl-type $f(Q,T)$
theory on these parameters. Moreover, we assess the stability of the proposed
model to ensure its viability as a cosmological scenario. Through our analysis,
we aim to gain insights into the potential implications and consequences of
Weyl-type $f(Q,T)$ gravity for bouncing scenarios, contributing to our
understanding of alternative gravitational theories in the context of
cosmology.
