“…For instance if, as we do in the following, we assume n = m = 1, Ω = I = ]α, β[, then one is led to the parabolic equation (1.2) u t = (φ (u x )) x , coupled with suitable boundary and initial conditions, which for smooth enough solutions u and provided that φ is smooth, takes the form u t = φ (u x )u xx ; such an equation has a forward-backward character depending on the sign of φ (u x ). A consequence of the ill-posedness of (1.2) is that, in spite of some interesting attempts, [33], [45], [37], [27], [26], [36], [31], there is not yet a satisfactory notion of weak solution which can adequately describe the rich phenomenology observed in numerical experiments [28], [41]. A natural approach in this situation is to associate with (1.2) a family of regular problems depending on a small parameter ε > 0 which are expected to approach (1.2) in the limit ε → 0 + , and try to define solutions to (1.2) as limits as ε → 0 + of solutions of the regularized problems, i.e.,…”