  Most cosmological models of inflation are far away from providing a smoking
gun at low energies. A model of Higgs inflation in the Next-to-Minimal
Supersymmetric Standard Model, however, changes the NMSSM phenomenology
drastically and may be well distinguished from the pure NMSSM or MSSM at a
future Linear Collider. We point out certain differences of the inflationary
model to the ordinary NMSSM and discuss the Higgs and neutralino/chargino
sector in particular to identify the smoking gun of inflation at electroweak
energies.
