
TL;DR
This paper explores the theoretical implications and potential future transition to an exactly supersymmetric universe within the string landscape multiverse, analyzing its properties and possible consequences.
Contribution
It provides preliminary estimates of the properties and implications of a future transition to an exactly supersymmetric universe in the string landscape framework.
Findings
Existence of a zero vacuum energy susy phase in string theory.
Potential consequences of transitioning to a susy universe.
Implications for the multiverse and cosmic evolution.
Abstract
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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