In this work, we study the problem of the reconstruction of the physics of inflation using current and future cosmological data from cosmic microwave background and gravitational waves experiments. In particular, we focus on the so-called (supergravity) α-attractor models of inflation constraining the shape of the potential as well as the reheating properties of the these models. Furthermore, we approach the problem of the reconstruction of the variation of the inflaton field during inflation providing a next order expression in terms of the inflationary variables.
Reconstruction of the physics of Inflation from next generation cosmological experiments
DI MARCO, ALESSANDRO
2018
Abstract
In this work, we study the problem of the reconstruction of the physics of inflation using current and future cosmological data from cosmic microwave background and gravitational waves experiments. In particular, we focus on the so-called (supergravity) α-attractor models of inflation constraining the shape of the potential as well as the reheating properties of the these models. Furthermore, we approach the problem of the reconstruction of the variation of the inflaton field during inflation providing a next order expression in terms of the inflationary variables.File in questo prodotto:
| File | Dimensione | Formato | |
|---|---|---|---|
|
Tesi dottorato Di Marco
accesso aperto
Licenza:
Tutti i diritti riservati
Dimensione
4.31 MB
Formato
Unknown
|
4.31 MB | Unknown | Visualizza/Apri |
I documenti in UNITESI sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
Utilizza questo identificativo per citare o creare un link a questo documento:
https://hdl.handle.net/20.500.14242/93526
Il codice NBN di questa tesi è
URN:NBN:IT:UNIROMA1-93526