On the Starobinsky model of inflation from supergravity
By F. Farakos, A. Kehagias, A. Riotto. 2013
222 citations recorded by the source corpus.
We discuss how the higher-derivative Starobinsky model of inflation originates from N=1N=1 supergravity. It is known that, in the old-minimal supergravity description written by employing a chiral compensator in the superconformal framework, the Starobinsky model is equivalent to a no-scale model with F-term potential. We show that the Starobinsky model can also be originated within the so-called new-minimal supergravity, where a linear compensator superfield is employed. In this formulation, the Starobinsky model is equivalent to standard supergravity coupled to a massive vector multiplet whose lowest scalar component plays the role of the inflaton and the vacuum energy is provided by a D-term potential. We also point out that higher-order corrections to the supergravity Lagrangian represent a threat to the Starobinsky model as they can destroy the flatness of the inflaton potential in its scalar field equivalent description.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Oceanography
View Paper: https://www.semanticscholar.org/paper/afbd27916ed93e6ce633b1cc7d809fa65bb2b315
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Citations in the corpus
- Cosmology with nilpotent superfields (2014, background): “There is an alternative class of models suggested by R+R supergravity in new minimal formulation [53] where the problem of moduli stabilization does not arise at all since the inflaton is the only scalar (member of a massive vector or tensor multiplet) but the Kähler manifold in which it is embedded”
- Inflationary Cosmology after Planck 2013 (2014, background): “In new minimal supergravity, R+R(2) models and their dual were given in [102, 103, 96, 104].”
- Minimal Supergravity Models of Inflation (2013, background): “In this respect, it is interesting that in the supergravity version of the theory R + γR2 developed in [11] the issue of stabilization of the extra moduli does not appear at all because this theory does not contain any other scalars except the inflaton [22].”
- A polynomial f(R) inflation model (2013, background): “The higher derivative terms may also originate from the supergravity [10, 11].”
- Multi-field conformal cosmological attractors (2013, result): “Recently another set of models with similar predictions was identified in [17–22], and some earlier works in the related area, such as [24,25], have been rediscovered and reinforced [6,19,21,23].”
- Exploring cosmic origins with CORE: Inflation (2016, methodology): “The Starobinsky model is currently the simplest among the inflationary models allowed by Planck data [3, 5, 205] and has been at the center stage of several theoretical developments in supergravity [78, 81, 82, 206], as explained in Section 2.”
- On sgoldstino-less supergravity models of inflation (2014, background): “A notable exception occurs in the models of D-term inflation with gauged shift symmetry [5–7], where the scalar partner of the inflaton is removed from the spectrum by a supersymmetric Higgs effect.”