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arXiv · hep-th/0611018

Meta-Stable Supersymmetry Breaking in a Cooling Universe

Willy Fischler·Vadim Kaplunovsky·Chethan Krishnan·Lorenzo Mannelli·Marcus Torres
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Abstract

We look at the recently proposed idea that susy breaking can be accomplished in a meta-stable vacuum. In the context of one of the simplest models (the Seiberg-dual of super-QCD), we address the following question: if we look at this theory as it cools from high temperature, is it at all possible that we can end up in a susy-breaking meta-stable vacuum? To get an idea about the answer, we look at the free energy of the system at high temperature. We conclude that the phase-structure of the free-energy as the temperature drops, is indeed such that there is a second order phase transition in the direction of the non-susy vacuum at a finite $T=T_c^Q$. On the other hand, the potential barrier in the direction of the susy vacuum is there all the way till $T \sim 0$.

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Willy Fischler, Vadim Kaplunovsky, Chethan Krishnan, Lorenzo Mannelli, Marcus Torres. 2007-02-28. Meta-Stable Supersymmetry Breaking in a Cooling Universe. https://doi.org/10.1088/1126-6708%2F2007%2F03%2F107

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