Neutrino Masses, Baryon Asymmetry, Dark Matter and the Moduli Problem : A Complete Framework
Piyush Kumar

TL;DR
This paper presents a comprehensive framework within string theory that addresses neutrino masses, baryon asymmetry, dark matter, and the moduli problem, proposing a consistent cosmological evolution post-inflation and before BBN.
Contribution
It introduces a realistic string compactification model that naturally generates baryon asymmetry and neutrino masses while solving the moduli problem with minimal MSSM extension.
Findings
Baryon asymmetry generated via Affleck-Dine leptogenesis after inflation.
Lightest neutrino is nearly massless in this framework.
Moduli and gravitino problems are naturally resolved.
Abstract
Recent developments in string theory have led to "realistic" string compactifications which lead to moduli stabilization while generating a hierarchy between the Electroweak and Planck scales at the same time. However, this seems to suggest a rethink of our standard notions of cosmological evolution after the end of inflation and before the beginning of BBN. We argue that within classes of realistic string compactifications, there generically exists a light modulus with a mass comparable to that of the gravitino which generates a large late-time entropy when it decays. Therefore, all known mechanisms of generating the baryon asymmetry of the Universe in the literature have to take this fact into account. In this work, we find that it is still possible to naturally generate the observed baryon asymmetry of the Universe as well as light left-handed neutrino masses from a period of…
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