Higgs-Squark-Slepton Inflation from the MSSM
arXiv:1912.07694 · doi:10.1103/PhysRevD.101.055027
Abstract
The inflation within the MSSM is proposed, where the inflaton field is a combination of the Higgs, squark and slepton states. While the inflationary phase is fully governed by the electron Yukawa superpotential coupling, the fields' condensates float along the flat -term trajectory. This predicts the MSSM parameter determined via the value of the curvature perturbation amplitude. The values of the scalar spectral index and the tensor-to-scalar ratio are predicted to be and . The postinflation reheating of the Universe proceeds by the radiative decay of the inflaton to the two gluons () with the reheating temperature GeV.
arXiv commentLaTex, 1 figure
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