Deforming the Starobinsky model in ghost-free higher derivative supergravities

G. A. Diamandis, B. C. Georgalas, K. Kaskavelis, A. B. Lahanas, and G. Pavlopoulos
Phys. Rev. D 96, 044033 – Published 24 August 2017

Abstract

We consider higher derivative supergravities that are dual to ghost-free N=1 supergravity theories in the Einstein frame. The duality is implemented by deforming the Kähler function, and/or the superpotential, to include nonlinear dependences on chiral fields that, in other approaches, play the role of the Lagrange multipliers employed to establish this duality. These models are of the no-scale type, and in the minimal case, they require the presence of four chiral multiplets, with a Kähler potential having the structure of the SU(4,1)/SU(4)×U(1) coset manifold. In the standard N=1 supergravity formulation, these models are described by a multifield scalar potential, featuring Starobinsky-like behavior in particular directions.

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  • Received 12 May 2017

DOI:https://doi.org/10.1103/PhysRevD.96.044033

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

G. A. Diamandis*, B. C. Georgalas, K. Kaskavelis, A. B. Lahanas§, and G. Pavlopoulos

  • National and Kapodistrian University of Athens, Department of Physics, Nuclear and Particle Physics Section, GR–157 71 Athens, Greece

  • *gdiam@phys.uoa.gr
  • vgeorgal@phys.uoa.gr
  • kkaskavelis@phys.uoa.gr
  • §alahanas@phys.uoa.gr
  • gepavlo@phys.uoa.gr

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Issue

Vol. 96, Iss. 4 — 15 August 2017

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