We quantitatively estimate the leading higher derivative corrections to N = 1 supergravity derived from IIB string compactifications and study how they may affect moduli stabilisation and LVS inflation models. Using the Kreuzer-Skarke database of 4D reflexive polytopes and their triangulated Calabi-Yau database, we present scanning results for a set of divisor topologies corresponding to threefolds with h1,1 between a and 5. In particular, we find several geometries suitable to realise blow-up inflation, fibre inflation and poly-instantons inflation, together with a classification of the divisors topologies for which the leading higher derivative corrections to the inflationary potential vanish. In all other cases, we instead estimate numerically how these corrections modify the inflationary dynamics, finding that they do not destroy the predictions for the main cosmological observables.
Cicoli, M., Licheri, M., Piantadosi, P., Quevedo, F., Shukla, P. (2024). Higher derivative corrections to string inflation. JOURNAL OF HIGH ENERGY PHYSICS, 2024(2), 0-40 [10.1007/jhep02(2024)115].
Higher derivative corrections to string inflation
Cicoli, MicheleMembro del Collaboration Group
;Licheri, Matteo
Membro del Collaboration Group
;Piantadosi, PellegrinoMembro del Collaboration Group
;
2024
Abstract
We quantitatively estimate the leading higher derivative corrections to N = 1 supergravity derived from IIB string compactifications and study how they may affect moduli stabilisation and LVS inflation models. Using the Kreuzer-Skarke database of 4D reflexive polytopes and their triangulated Calabi-Yau database, we present scanning results for a set of divisor topologies corresponding to threefolds with h1,1 between a and 5. In particular, we find several geometries suitable to realise blow-up inflation, fibre inflation and poly-instantons inflation, together with a classification of the divisors topologies for which the leading higher derivative corrections to the inflationary potential vanish. In all other cases, we instead estimate numerically how these corrections modify the inflationary dynamics, finding that they do not destroy the predictions for the main cosmological observables.File | Dimensione | Formato | |
---|---|---|---|
JHEP02(2024)115.pdf
accesso aperto
Tipo:
Versione (PDF) editoriale
Licenza:
Licenza per Accesso Aperto. Creative Commons Attribuzione (CCBY)
Dimensione
953.08 kB
Formato
Adobe PDF
|
953.08 kB | Adobe PDF | Visualizza/Apri |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.