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The Hubble parameter during the inflationary era must be smaller than thegravitino mass if the moduli are stabilized by the Kachru-Kallosh-Linde-Trivedimechanism. This condition represents the difficulty to combine the low scaleSUSY breaking and the high scale inflation. We propose a simple mechanism whichcan naturally separate the inflation scale from the SUSY breaking scale today.

Instant uplifted inflation: A solution for a tension between inflation and SUSY breaking scale