A very important open question related to the pygmy dipole resonance is about its quite elusive collective nature. In this paper, within a harmonic oscillator shell model, generalizing an approach introduced by Brink, we first identify the dipole normal modes in neutron rich nuclei and derive the energy weighted sum rule exhausted by the pygmy dipole resonance. Then solving numerically the self-consistent Landau-Vlasov kinetic equations for neutrons and protons with specific initial conditions, we explore the structure of the different dipole vibrations in the 132 Sn system and investigate their dependence on the symmetry energy. We evidence the existence of a distinctive collective isoscalar-like mode with an energy well below the Giant Dipole Resonance (GDR), very weakly dependent on the isovector part of the nuclear effective interaction. At variance the corresponding strength is rather sensitive to the behavior of the symmetry energy below saturation, which rules the number of excess neutrons in the nuclear surface. PACS numbers: 25.70.Pq, 25.70.Mn, 21.65.Ef, 24.10.Cn Keywords:One of the important tasks in many-body physics is to understand the emergence of the collective features as well as their structure in terms of the individual motion of the constituents. The steady progress of experimental methods of investigation opens now the possibility to study very neutron rich nuclei, beyond the limits of stability. The goal is to have a unified picture of the evolution of various nuclear properties with mass and isospin and to test the validity of our theoretical understanding over an extended domain of analysis.New exotic collective excitations show up when one moves away from the valley of stability [1]. Their experimental characterization and theoretical description is a challenge for modern nuclear physics. Recent experiments provided several evidences about their existence but the available information is still incomplete and their nature is a matter of debate.An interesting exotic mode is the Pygmy Dipole Resonance (PDR) which was observed as an unusually large concentration of the dipole response at energies clearly below the values associated with the GDR. The latter is one of the most prominent and robust collective motions, present in all nuclei, whose centroid position varies, for medium-heavy nuclei, as 80A −1/3 M eV . Adrich et al. [2] reported the observation of a resonant-like shape distribution with a pronounced peak around 10M eV in 130 Sn and 132 Sn isotopes. A concentration of dipole excitations near and below the particle emission threshold was also observed in stable Sn nuclei, a systematics of PDR in these systems being presented in [3]. It was concluded that the strongest transitions locate at energies between 5 and 8.5M eV and a sizable fraction of the Energy-Weighted Sum Rule (EWSR) is exhausted by these states. From a comparison of the available data for stable and unstable Sn isotopes a correlation between the fraction of pygmy strength and isospin asymmetry was noted [4]. In general t...