Supersymmetric Sneutrino-Higgs Inflation
arXiv:1606.00431 · doi:10.1016/j.physletb.2016.09.059
Abstract
It is shown that in the phenomenologically realistic supersymmetric MSSM theory, a linear combination of the neutral, up Higgs field with the third family left-and right-handed sneutrinos can play the role of the cosmological inflaton. Assuming that supersymmetry is softly broken at a mass scale of order , the potential energy associated with this field allows for 60 e-foldings of inflation with the cosmological parameters being consistent with all Planck2015 data. The theory does not require any non-standard coupling to gravity and the physical fields are all sub-Planckian during the inflationary epoch. It will be shown that there is a "robust" set of initial conditions which, in addition to satisfying the Planck data, simultaneously are consistent with all present LHC phenomenological requirements.
15 pages, 3 figures. Version 2: Updated to be consistent with journal version, includes new references and other minor changes
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- The -parity Violating Decays of Charginos and Neutralinos in the B-L MSSM
- Sneutrino driven GUT Inflation in Supergravity
- Gravitino Dark matter, Non Thermal Leptogenesis and Low reheating temperature in No-scale Higgs Inflation
- Non-vanishing Heterotic Superpotentials on Elliptic Fibrations
- No-scale SUGRA Inflation and Type-I seesaw
- Bayesian naturalness, simplicity, and testability applied to the MSSM GUT
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- FIMP Dark Matter in Heterotic M-Theory