On the robustness of the primordial power spectrum in renormalized Higgs inflation

We study the cosmological consequences of higher-dimensional operators respecting the asymptotic symmetries of the tree-level Higgs inflation action. The main contribution of these operators to the renormalization group enhanced potential is localized in a compact field range, whose upper limit is c...

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Hauptverfasser: Bezrukov, Fedor (VerfasserIn) , Pauly, Martin (VerfasserIn) , Rubio, Javier (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 20 February 2018
In: Journal of cosmology and astroparticle physics
Year: 2018, Heft: 2, Pages: ?
ISSN:1475-7516
DOI:10.1088/1475-7516/2018/02/040
Online-Zugang:Verlag, Volltext: https://doi.org/10.1088/1475-7516/2018/02/040
Verlag, Volltext: https://doi.org/10.1088%2F1475-7516%2F2018%2F02%2F040
Volltext
Verfasserangaben:Fedor Bezrukov, Martin Pauly and Javier Rubio
Beschreibung
Zusammenfassung:We study the cosmological consequences of higher-dimensional operators respecting the asymptotic symmetries of the tree-level Higgs inflation action. The main contribution of these operators to the renormalization group enhanced potential is localized in a compact field range, whose upper limit is close to the end of inflation. The spectrum of primordial fluctuations in the so-called universal regime turns out to be almost insensitive to radiative corrections and in excellent agreement with the present cosmological data. However, higher-dimensional operators can play an important role in critical Higgs inflation scenarios containing a quasi-inflection point along the inflationary trajectory. The interplay of radiative corrections with this quasi-inflection point may translate into a sizable modification of the inflationary observables.
Beschreibung:Gesehen am 19.08.2019
Beschreibung:Online Resource
ISSN:1475-7516
DOI:10.1088/1475-7516/2018/02/040