Model with two periods of inflation
A scenario with two subsequent periods of inflationary expansion in the very early Universe is examined. The model is based on a potential motivated by symmetries being found in field theory at high energy. For various parameter sets of the potential, the spectra of scalar and tensor perturbations t...
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
5 January 2016
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| In: |
Physical review
Year: 2016, Jahrgang: 93, Heft: 2 |
| ISSN: | 2470-0029 |
| DOI: | 10.1103/PhysRevD.93.025001 |
| Online-Zugang: | Resolving-System, lizenzpflichtig, Volltext: https://doi.org/10.1103/PhysRevD.93.025001 Verlag, lizenzpflichtig, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.93.025001 
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| Verfasserangaben: | Simon Schettler and Jürgen Schaffner-Bielich |
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A model with two periods of inflation
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