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Properties of a future susy universe
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In the string landscape picture, the effective potential is characterized by an enormous number of local minima of which only a minuscule fraction are suitable for the evolution of life. In this "multiverse", random transitions are continually made between the various minima with the most likely transitions being to minima of lower vacuum energy. The inflationary era in the very early universe ended with such a transition to our current phase which is described by a broken supersymmetry and a small, positive vacuum energy. However, it is likely that an exactly supersymmetric (susy) phase of zero vacuum energy as in the original superstring theory also exists and that, at some time in the future, there will be a transition to this susy world. In this article we make some preliminary estimates of the consequences of such a transition.
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Cited by 1 Pith paper
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Extending the susy model to core-collapse supernovae
With one new tuned parameter, the paper claims a single supersymmetric phase transition can explain both Type Ia and core-collapse supernovae, heavy element production, and the black hole mass gap.
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