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- W2022163534 abstract "It has been demonstrated that fluctuations in the new inflationary universe may be almost scale-invariant, but are unfortunately too large. We show that supersymmetric inflationary models allow the fluctuations to be smaller. In a toy supersymmetric model, the perturbations are O(10−4) is the Yukawa interactions are O(10−6μmp) where μ is the magnitude of the Higgs vacuum expectation value driving the inflation. It is therefore easier to have small fluctuations if inflation occurs close to the Planck epoch." @default.
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- W2022163534 date "1983-01-01" @default.
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- W2022163534 title "Fluctuations in a supersymmetric inflationary universe" @default.
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- W2022163534 doi "https://doi.org/10.1016/0370-2693(83)90456-2" @default.
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