Dynamical complexity of the Teleparallel gravity cosmology
  The exploration of teleparallel gravity has been done from a dynamical
systems point of view in order to be tested against the cosmological evolution
currently observed. So far, the proposed autonomous systems have been
restrictive over a constant dynamical variable, which contains information
related to the dynamics on the $H_0$ value. It is therefore that in this paper
we consider a generalization of the dynamical system by imposing a nonconstant
degree of freedom over it which allows us to rewrite a generic autonomous
dynamical analysis. We describe the treatment of our nonlinear autonomous
system by studying the hyperbolic critical points and discuss an interesting
phenomenological feature in regards to $H_0$: the possibility to obtain a
best-fit value for this parameter in a cosmologically viable $f(T,B)$ model, a
mixed power law. This result allows us to present a generic scenario in which
it is possible to fix constraints to solve the $H_0$ tension at late times
where its linearized solutions are considered.
