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Dynamics of O(N) chiral supersymmetry at finite energy density
Authors:J Baacke  D Cormier  H J de Vega  K Heitmann  
Institution:

a Institut für Physik, Universität Dortmund, D-44221 Dortmund, Germany

b Centre for Theoretical Physics, Sussex University, Falmer, Brighton, BN1 9QH, England, UK

c Laboratoire de Physique Théorique et Hautes Energies, Université Pierre et Marie Curie (Paris VI), Tour 16, 1er. étage, 4, Place Jussieu, 75252 Paris, Cedex 05, France

d T-8, Theoretical Division, MS B285, Los Alamos National Laboratory, Los Alamos, NM 87545, USA

Abstract:We consider an O(N) version of a massive, interacting, chiral supersymmetry model solved exactly in the large N limit. We demonstrate that the system approaches a stable attractor at high energy densities, corresponding to a non-perturbative state for which the relevant field quanta are massless. The state is one of spontaneously broken O(N), which, due to the influence of supersymmetry, does not become restored at high energies. Introducing soft supersymmetry breaking to the Lagrangian results in scalar masses at the soft breaking scale ms independent of the mass scale of supersymmetry μ, with even smaller masses for the fermions.
Keywords:
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