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• W3100906946 endingPage "046" @default.
• W3100906946 startingPage "046" @default.
• W3100906946 abstract "Modular cosmology is plagued by overproduction of unwanted relics, gravitinos and especially moduli, at relatively low energy scales. Thermal inflation provides a compelling solution to this moduli problem, but invalidates most baryogenesis scenarios. We propose a simple model in which the MSSM plus neutrino mass term (LHu)2is supplemented by a minimal flaton sector to drive the thermal inflation, and make two crucial assumptions: the flaton vacuum expectation value generates the μ-term of the MSSM and mL2+mHu2 < 0. The second assumption is particularly interesting in that it violates a well known constraint, implying that there exists a nearby deep non-MSSM vacuum, and provides a clear signature of our model which can be tested at future particle accelerators. We show that our model leads to thermal inflation followed by Affleck-Dine leptogenensis along the LHuflat direction. A key feature of our leptogenesis scenario is that the HuHdflat direction is also induced to temporarily acquire a large value, playing a crucial role in the leptogenesis, as well as dynamically shielding the field configuration from the deep non-MSSM minimum, ensuring that the fields relax into our MSSM vacuum." @default.
• W3100906946 created "2020-11-23" @default.
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• W3100906946 creator A5022567298 @default.
• W3100906946 creator A5036860760 @default.
• W3100906946 creator A5047914486 @default.
• W3100906946 date "2004-11-17" @default.
• W3100906946 modified "2023-09-25" @default.
• W3100906946 title "Modular Cosmology, Thermal Inflation, Baryogenesis and Predictions for Particle Accelerators" @default.
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• W3100906946 doi "https://doi.org/10.1088/1126-6708/2004/11/046" @default.
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