We study chiral symmetry breaking in the Nambu-Jona-Lasinio model regularized in propertime in arbitrary space-time dimensions through an iterative procedure by writing the gap equation in the form of a discrete dynamical system with the coupling constant as the control parameter. Expectedly, we obtain the critical coupling for chiral symmetry breaking when a nontrivial solution bifurcates away from the trivial one and becomes an attractor. By increasing further the value coupling constant, we observe a second bifurcation where the dynamical solution is no longer an attractor, and observation that holds true in all space-time dimensions. In the super-strong coupling regime, the system becomes chaotic.Quantum chromodynamics (QCD) [1,2] is nowadays accepted to be the theory that describes strong interactions among quarks and gluons. It possesses two important and opposite features, asymptotic freedom [1] in the high energy domain, where quarks move freely at short distances. Perturbative QCD is the appropriate framework to approach this regime. On the other hand, there exists quark confinement [3] in the low-energy and largedistances regime. In this case, the fundamental degrees of freedom bind in hadronic bound-states (mesons, baryons and exotic), the coupling becomes strong and the theory highly non-linear. A number of non-perturbative frameworks have been developed to study low-energy QCD, among which we find Lattice QCD [4], Schwinger-Dyson equations (SDEs) [5,6] (see for reviews of SDEs in hadron physics) and other field-theoretical approaches, like the functional renormalization group [14-16], as well as effective models. Nambu-Jona-Lasinio (NJL) model [17,18] is a favorite one to study the properties of hadrons mostly in connection with chiral symmetry breaking (see, for instance, the reviews in Refs. [19,20]), and it is the general topic of this article. The model is non-renormalizable and thus, there are several schemes in which the regulator and coupling are selected to match static properties of pions (see, for example, Ref. [21]). Here, we select to regulate the gap equation in the proper-time (PT) scheme. Momentum integrals become Gaussian and thus are readily performed; the regulator comes in the PT integration, as opposed to the more frequently employed hard momentum cutoff regularization scheme [22] (the UV regulator in momentum space in the latter case is identified with the IR cut-off in proper-time integrals). Furthermore, by introducing an IR cut-off in momentum (UV in PT), we mimic confinement in the model [23][24][25]; the second cut-off removes quark-antiquark production thresholds, in the deep infra-red region of the quark propagator. This procedure has an added advantage that the resulting quark propagator naturally fulfills the Axial-Vector Ward identities for bound states. Furthermore, the PT regularization scheme allows an easy incorpora-tion of plasma effects, including finite temperature, density and external magnetic fields. Among other things, these extreme conditions make the effec...