Gravity mediation without a Polonyi problem
Kazunori Nakayama, Fuminobu Takahashi, Tsutomu T. Yanagida

TL;DR
This paper proposes a solution to the cosmological Polonyi problem in high-scale SUSY models with a 125GeV Higgs, enabling successful leptogenesis by enhancing Polonyi-inflaton coupling.
Contribution
It introduces a mechanism to solve the Polonyi problem by increasing the Polonyi-inflaton coupling, allowing high-scale SUSY models to be cosmologically viable.
Findings
Polonyi problem can be mitigated with enhanced coupling
Leptogenesis scenarios remain viable in this framework
High-scale SUSY models compatible with cosmology
Abstract
Recent indications of the 125GeV Higgs at the LHC can be explained in a relatively high-scale SUSY scenario where the sparticle masses are multi-TeV as is realized in the focus-point region. However, it suffers from the notorious cosmological Polonyi problem. We argue that the Polonyi problem is solved and thermal or non-thermal leptogenesis scenario works successfully, if a certain Polonyi coupling to the inflaton is enhanced by a factor of 10-100.
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