Abstract

We propose a supersymmetrisation of the cosmological constant in ordinary N=1 supergravity that breaks supersymmetry spontaneously by a constant Fayet-Iliopoulos (FI) term associated to a U(1) symmetry. This term is a variation of a new gauge invariant FI term proposed recently, which is invariant under Kähler transformations and can be written even for a gauged R-symmetry on top of the standard FI contribution. The two terms are the same in the absence of matter but differ in its presence. The proposed term is reduced to a constant FI-term up to fermion interactions that disappear in the unitary gauge in the absence of any F-term supersymmetry breaking. The constant FI term leads to a positive cosmological constant, uplifting the vacuum energy from the usual anti-de Sitter supergravity to any higher value.

Highlights

  • It is well known that the cosmological constant in supergravity is highly constrained

  • We propose a supersymmetrisation of the cosmological constant in ordinary N = 1 supergravity that breaks supersymmetry spontaneously by a constant FayetIliopoulos (FI) term associated to a U (1) symmetry

  • The proposed term is reduced to a constant FI-term up to fermion interactions that disappear in the unitary gauge in the absence of any F-term supersymmetry breaking

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Summary

Introduction

It is well known that the cosmological constant in supergravity is highly constrained. We propose a modification/generalisation of this FI term that has the following properties: (1) it can be written independently whether the corresponding U (1) gauges or not the R-symmetry; (2) in the absence of matter fields and in the case of an ordinary (non-R) U (1), it coincides with the one proposed in [8]; (3) in the case of a U (1)R, it can be written on top of the standard constant FI term; (4) in the presence of matter fields the action is invariant under Kähler transformations and its bosonic contribution is always a constant FI term that uplifts in particular the vacuum energy by an arbitrary positive constant. We have two appendices; “Appendix A” contains useful formulae used in the text, while in “Appendix B” we compute the fermionic part of the supergravity action

Review and definitions
Kähler invariant generalization of the new FI term
A constant FI contribution to the scalar potential
Conclusions
Covariant derivatives
Multiplication laws
B Fermion couplings
Full Text
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