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Reheating and geometrical destabilisation in Fibre Inflation

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Reheating and geometrical destabilisation in Fibre Inflation
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20
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You are free to use, copy, distribute and transmit the work or content in unchanged form for any legal and non-commercial purpose as long as the work is attributed to the author in the manner specified by the author or licensor.
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I will focus on type IIB Fibre Inflation and discuss first the interplay between reheating and the production of axionic dark radiation after the end of inflation. I will then analyse the possibility to have a potentially dangerous geometrical destabilisation of ultra-light isocurvature modes.