Quintessential inflation with dynamical Higgs generation as an affine gravity

  • First, we propose a scale-invariant modified gravity interacting with a neutral scalar inflaton and a Higgs-like SU(2)×U(1) iso-doublet scalar field based on the formalism of non-Riemannian (metric-independent) spacetime volume-elements. This model describes, in the physical Einstein frame, a quintessential inflationary scenario driven by the “inflaton” together with the gravity-“inflaton” assisted dynamical spontaneous SU(2)×U(1) symmetry breaking in the post-inflationary universe, whereas the SU(2)×U(1) symmetry remains intact in the inflationary epoch. Next, we find the explicit representation of the latter quintessential inflationary model with a dynamical Higgs effect as an Eddington-type purely affine gravity.

Download full text files

Export metadata

Additional Services

Share in Twitter Search Google Scholar
Metadaten
Author:David BenistyORCiD, Eduardo I. Guendelman, Emil Nissimov, Svetlana Pacheva
URN:urn:nbn:de:hebis:30:3-546577
DOI:https://doi.org/10.3390/sym12050734
ISSN:2073-8994
Parent Title (English):Symmetry
Publisher:MDPI
Place of publication:Basel
Document Type:Article
Language:English
Date of Publication (online):2020/05/05
Date of first Publication:2020/05/05
Publishing Institution:Universitätsbibliothek Johann Christian Senckenberg
Release Date:2020/06/12
Tag:dark energy; dynamical Higgs effect; inflation; quintessence
Volume:12
Issue:734
Page Number:16
HeBIS-PPN:467145989
Institutes:Physik / Physik
Wissenschaftliche Zentren und koordinierte Programme / Frankfurt Institute for Advanced Studies (FIAS)
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Sammlungen:Universitätspublikationen
Licence (German):License LogoCreative Commons - Namensnennung 4.0