gravity and the standard σ-models well understood in the literature. This issue explains why
there are two non-trivial family of solutions for the spherically symmetric case inside the non-
linear massive gravity formulations with two free parameters α and β. In general, the case
$\beta<\alpha^ 2$ has a single physical vacuum state. On the other hand, the case
$\beta=\alpha^ 2$ contains a natural vacuum degeneracy. This is in perfect analogy with the …