For scalar-tensor teleparallel dark energy with f(phi) proportional to (phi+c)^2 and V(phi) proportional to f(phi)^lambda, a viable trajectory needs lambda much greater than 1 and zeta^2 much less than 1.
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Constraining cosmological dynamics of scalar-tensor models of dark energy in teleparallel gravity
For scalar-tensor teleparallel dark energy with f(phi) proportional to (phi+c)^2 and V(phi) proportional to f(phi)^lambda, a viable trajectory needs lambda much greater than 1 and zeta^2 much less than 1.