Abstract:We propose a four-dimensional N = 1 supergravity-based Starobinsky-type inflationary model in terms of a single massive vector multiplet, whose action includes the Dirac-Born-Infeld-type kinetic terms and a generalized (new) Fayet-Iliopoulos-type term, without gauging the R-symmetry. The bosonic action and the scalar potential are computed. The inflaton is the superpartner of the Goldstino in our model, and supersymmetry is spontaneously broken after inflation by the D-type mechanism, whose scale is related to… Show more
“…New Fayet-Iliopoulos terms have been recently introduced for N = 1 supergravity theories that do not require the gauging of the R-symmetry [22][23][24][25], and have been studied and developed in a series of publications [71][72][73][74][75][76][77][78]. To highlight some interesting aspects of these constructions let us mention that new type of scalar potentials can be introduced that lead to new possibilities for inflation in supergravity [24,72], but also to new possibilities regarding the vacuum structure [22,25], while the matter content of the theory is still described by standard N = 1 supermultiplets, including the FI gauge multiplet.…”
We present a new type of Fayet-Iliopoulos (FI) terms in N = 2 supergravity that do not require the gauging of the R-symmetry. We elaborate on the impact of such terms on the vacuum structure of the N = 2 theory and compare their properties with the standard Fayet-Iliopoulos terms that arise from gaugings. In particular, we show that, with the use of the new FI terms, models with a single physical N = 2 vector multiplet can be constructed that give stable de Sitter vacua.1 See for instance [3-8] for reviews.
“…New Fayet-Iliopoulos terms have been recently introduced for N = 1 supergravity theories that do not require the gauging of the R-symmetry [22][23][24][25], and have been studied and developed in a series of publications [71][72][73][74][75][76][77][78]. To highlight some interesting aspects of these constructions let us mention that new type of scalar potentials can be introduced that lead to new possibilities for inflation in supergravity [24,72], but also to new possibilities regarding the vacuum structure [22,25], while the matter content of the theory is still described by standard N = 1 supermultiplets, including the FI gauge multiplet.…”
We present a new type of Fayet-Iliopoulos (FI) terms in N = 2 supergravity that do not require the gauging of the R-symmetry. We elaborate on the impact of such terms on the vacuum structure of the N = 2 theory and compare their properties with the standard Fayet-Iliopoulos terms that arise from gaugings. In particular, we show that, with the use of the new FI terms, models with a single physical N = 2 vector multiplet can be constructed that give stable de Sitter vacua.1 See for instance [3-8] for reviews.
“…The authors are grateful to Hiroyuki Abe for his collaboration on related work in Refs. [23,28] and Sergei Kuzenko for correspondence. S.A. was supported in part by a Waseda University Grant for Special Research Projects (Project number: 2019E-059).…”
Section: Acknowledgementsmentioning
confidence: 99%
“…[18,19]. The viable SSB after the Starobinsky inflation, which gives rise to an adjustable (or observable) cosmological constant, is also possible by the use of the alternative Fayetlliopoulos (FI) terms without the gauging of the R-symmetry [20,21,22,23]. However, an origin of those FI terms in string theory and a restoration of another supersymmetry are still unclear, see e.g., Refs.…”
Section: Introductionmentioning
confidence: 99%
“…Though we did our calculations with the DBI kinetic terms for the vector multiplet, in this paper we only use the Maxwell-type kinetic terms for simplicity, because the DBI structure does not significantly affect the Starobinsky inflation and the moduli stabilization in question, according to our findings (see also Refs. [18,23,28] for more).…”
The minimal Starobinsky supergravity with inflaton (scalaron) and goldstino in a massive vector supermultiplet is coupled to the dilaton-axion chiral superfield with the no-scale Kähler potential and a superpotential. The Kachru-Kallosh-Linde-Trivedi (KKLT)-type superpotential with a constant term is used to stabilize dilaton and axion during inflation, but it is shown to lead to an instability. The instability is cured by adding the alternative Fayet-Iliopoulos (FI) term that does not lead to the gauged R-symmetry. Other stabilization mechanisms, based on the Wess-Zumino (WZ)-type superpotential, are also studied in the presence of the FI term. A possible connection to the D3-brane models is briefly discussed too.
“…In the literature there have appeared various applications of the generalised FI terms [21,22,23,24,25,26,27,28,29,30,31], including inflationary cosmological models.…”
As an extension of the recent construction of generalised Fayet-Iliopoulos terms in N = 1 supergravity given in [1], we present self-interactions for a vector multiplet coupled to conformal supergravity. They are used to construct new models for spontaneously broken local supersymmetry.
VThe super-Weyl invariance of V (n) follows from the discussion in [10] (see also [11]).Associated with V (n) is the following generalised FI term [1]
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