On stable non supersymmetric vacua at the bottom of cascading theories

We consider a wide class of cascading gauge theories which usually lead to runaway behaviour in the IR, and discuss possible deformations of the superpotential at the bottom of the cascade which stabilize the runaway direction and provide stable non-supersymmetric vacua. The models we find may allow for a weakly coupled supergravity analysis of dynamical supersymmetric breaking in the context of the gauge/string correspondence. © SISSA 2006.

Vietnam’s political economy: a discussion on the 1986-2016 period

Being a member of the thriving ASEAN and successfully implementing economic renovation (Doi Moi) have drawn the world's attention on Vietnam around the turn of the millennium. Some even expected a much faster pace of transformation, and renewed economic, AND political, reforms in Vietnam, or Doi Moi II.However, in the recent transition turmoil the Vietnamese economy has experienced some significant setback, and the solution for getting the country out of the downward spiral of low productivity, waning purchasing power and increasing costs of doing business cannot be worked out without addressing those political economy issues that have shaped the modus operandi of the nation's economic system. This article discusses the post-Doi Moi political economy in Vietnam, from 1986 to 2016 – when the 12th Congress of the Communist Party of Vietnam takes place – and prospects of reviving reform momentum in subsequent years.

Consistent deformations of [p,p]-type gauge field theories

Using BRST-cohomological techniques, we analyze the consistent deformations of theories describing free tensor gauge fields whose symmetries are represented by Young tableaux made of two columns of equal length p, p > 1. Under the assumptions of locality and Poincaré invariance, we find that there is no consistent deformation of these theories that non-trivially modifies the gauge algebra and/or the gauge transformations. Adding the requirement that the deformation contains no more than two derivatives, the only possible deformation is a cosmological-constant-like term. © SISSA/ISAS 2004.