The populist re-politicization : some lessons from South America and Southern Europe

This article proposes an alternative categorization of the populist phenomena, by elaborating the distinction between electoral-delegative and participative-mobilising populisms. All the populist phenomena share some common traits, such as a polarising and antagonist discourse dividing the society into a "People" and some "elites" or privileged sectors, their reliance on a strong leadership, a pretension to be majoritarian and to achieve the power at the national level in order to restore the sovereignty of the People. Nonetheless, the strategies for achieving these goals vary according to the specific diagnoses that would correct the perceived deficiencies of the representative democracies in terms of accountability of the representatives. The populisms closer to the electoral-delegative pole stress the symbolic dimension of the concept of representation, thus relying on a strong leader able to "truly interpret" the general will of the People. Those closer to the participative-mobilising pole call for an active involvement of the People in the decision-making process in order to effectively control the public institutions, stressing the descriptive dimension of the concept of representation and sometimes questioning the theoretical bases sustaining the representative democracy. I provide a brief discussion on four participative-mobilising populist experiences, i.e. the MAS-IPSP, the Kirchnerism, the M5S and Podemos, focusing on their internal organizations and relying on an extensive fieldwork (consisting in one hundred in-depth interviews with country experts and party's representatives at regional and national levels) that I conducted for a broader research project

Scaling relations of supersonic turbulence in star-forming molecular clouds

We present a direct numerical and analytical study of driven supersonic MHD turbulence that is believed to govern the dynamics of star-forming molecular clouds. We describe statistical properties of the turbulence by measuring the velocity difference structure functions up to the fifth order. In particular, the velocity power spectrum in the inertial range is found to be close to E(k) \~ k^{-1.74}, and the velocity difference scales as ~ L^{0.42}. The results agree well with the Kolmogorov--Burgers analytical model suggested for supersonic turbulence in [astro-ph/0108300]. We then generalize the model to more realistic, fractal structure of molecular clouds, and show that depending on the fractal dimension of a given molecular cloud, the theoretical value for the velocity spectrum spans the interval [-1.74 ... -1.89], while the corresponding window for the velocity difference scaling exponent is [0.42 ... 0.78].Comment: 17 pages, 6 figures include