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- W2116052157 abstract "We describe a simple and predictive scenario for baryogenesis in theories with large extra dimensions which resembles Affleck-Dine baryogenesis. The Affleck-Dine field is a complex scalar field carrying a $U(1)_{chi}$ charge which is dynamically broken after the end of inflation. This generates an excess of $chi$ over $bar chi$, which then decays into Standard Model fermions to produce an excess of baryons over anti-baryons. Our model is very constrained because the Affleck-Dine field has to be sufficiently flat during inflation. It is also a source for density fluctuations which can be tested in the coming satellite and balloon experiments." @default.
- W2116052157 created "2016-06-24" @default.
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- W2116052157 date "2001-12-01" @default.
- W2116052157 modified "2023-09-24" @default.
- W2116052157 title "Baryogenesis in theories with large extra spatial dimensions" @default.
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- W2116052157 doi "https://doi.org/10.1016/s0550-3213(01)00474-6" @default.
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