| Preprint/Report | PUBDB-2018-00642 |
2018
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Please use a persistent id in citations: doi:10.3204/PUBDB-2018-00642
Report No.: DESY-18-005; arXiv:1801.04256
Abstract: 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.
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