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The Dark Universe after Reheating in String Inflation
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The Dark Universe after Reheating in String Inflation
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We study the production of dark matter and dark radiation after reheating in string inflation models where the Calabi-Yau has a fibred structure and the visible sector lives on D3 branes. We show how the interplay between different physical constraints from inflation, reheating, supersymmetry breaking and dark radiation, leads to distinct predictions for the nature of dark matter.
Forward citations
Cited by 2 Pith papers
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