Dark matter via Baryogenesis: Affleck-Dine Mechanism in the Minimal Supersymmetric Standard Model

K. El Bourakadi; M. Ferricha-Alami; Z. Sakhi; M. Bennai; H. Chakir

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arXiv · 2307.15541

Dark matter via Baryogenesis: Affleck-Dine Mechanism in the Minimal Supersymmetric Standard Model

K. El Bourakadi·M. Ferricha-Alami·Z. Sakhi·M. Bennai·H. Chakir

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Abstract

We conducted an investigation into Affleck-Dine baryogenesis within the context of D-term inflation, specifically focusing on its relationship with a recent reheating formalism. It was found that by considering a specific reheating temperature, the observed baryon asymmetry can be accounted through Affleck-Dine baryogenesis. Additionally, the majority of gravitinos are inferred to be generated from the decay of the next-to-lightest supersymmetric particle, with Q-balls potentially serving as a source of gravitinos via NSP decay. The temperature at which decay occurs depends on the charge of the Q-balls, which is determined by the fragmentation of the Affleck-Dine condensate. Remarkably, the gravitino mass required for dark matter aligns naturally with the theoretical gravitino mass.

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K. El Bourakadi, M. Ferricha-Alami, Z. Sakhi, M. Bennai, H. Chakir. 2023-07-28. Dark matter via Baryogenesis: Affleck-Dine Mechanism in the Minimal Supersymmetric Standard Model. https://arxiv.org/abs/2307.15541

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