Origin of Structure in a Supersymmetric Quantum Universe
classification
🌀 gr-qc
astro-phhep-th
keywords
quantumsupersymmetricmodelperturbationsadvancecosmologicalcurrentdensity
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In this report we advance the current repertoire of quantum cosmological models to incorporate inhomogenous field modes in a supersymmetric manner. In particular, we introduce perturbations about a supersymmetric FRW model. A quantum state of our model has properties typical of the no-boundary (Hartle--Hawking) proposal. This solution may then lead to a scale--free spectrum of density perturbations.
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