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dc.contributor.authorPallis, Constantinosen
dc.contributor.authorToumbas, Nicolaos K.en
dc.creatorPallis, Constantinosen
dc.creatorToumbas, Nicolaos K.en
dc.date.accessioned2019-12-02T15:32:16Z
dc.date.available2019-12-02T15:32:16Z
dc.date.issued2016
dc.identifier.issn1475-7516
dc.identifier.urihttp://gnosis.library.ucy.ac.cy/handle/7/58965
dc.description.abstractWe present a novel realization of Starobinsky-type inflation within Supergravity using two chiral superfields. The proposed superpotential is inspired by induced-gravity models. The Kähler potential contains two logarithmic terms, one for the inflaton T and one for the matter-like field S, parameterizing the SU(1,1)/U(1) × SU(2)/U(1) Kähler manifold. The two factors have constant curvatures -m/n and 2/n2, where n, m are the exponents of T in the superpotential and Kähler potential respectively, and 0 < n2 ≤ 6. The inflationary observables depend on the ratio 2n/m only. Essentially they coincide with the observables of the original Starobinsky model. Moreover, the inflaton mass is predicted to be 3·1013 GeV.en
dc.sourceJournal of Cosmology and Astroparticle Physicsen
dc.source.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-84969974195&doi=10.1088%2f1475-7516%2f2016%2f05%2f015&partnerID=40&md5=4843296961026f278c535107f9059bb4
dc.subjectinflationen
dc.subjectsupersymmetry and cosmologyen
dc.titleStarobinsky-type inflation with products of Kähler manifoldsen
dc.typeinfo:eu-repo/semantics/article
dc.identifier.doi10.1088/1475-7516/2016/05/015
dc.description.volume2016
dc.description.issue05
dc.description.startingpage015.1
dc.description.endingpage015.19
dc.author.facultyΣχολή Θετικών και Εφαρμοσμένων Επιστημών / Faculty of Pure and Applied Sciences
dc.author.departmentΤμήμα Φυσικής / Department of Physics
dc.type.uhtypeArticleen
dc.description.notes<p>Cited By :2</p>en
dc.source.abbreviationJ.Cosmol.Astroparticle Phys.en
dc.contributor.orcidToumbas, Nicolaos K. [0000-0001-8879-7330]
dc.gnosis.orcid0000-0001-8879-7330


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