Relaxed Supergravity

Abstract

We propose a novel class of N = 1 supergravity (called "Relaxed supergravity") that can enlarge the space of scalar potentials, relaxing the strongly-constrained form of the prototype supergravity potential. It has very long been considered that in N = 1 supergravity a negative term of scalar potential can be given only by the gravitino-mass term (i.e. −3e G ) from the F-term potential, while such negative term is absent in global supersymmetry (SUSY). In this letter, however, we firstly discover a new negative-definite contribution to the scalar potential in N = 1 supergravity and even global SUSY. In the end, this allows us to have a general scalar potential. To achieve this, we start with detection of a "no-go" theorem for the higher order corrections in minimal supergravity models of inflation, which was investigated by Ferrara, Kallosh, Linde, and Porrati (FKLP). Based on the no-go theorem, we establish a superconformal action of a certain higher order correction for generating the new negative term. Then, we identify essential constraints on the new negative term by inspecting the suppression of the nonrenormalizable terms. We find that relaxed supergravity has a cutoff equal to SUSY breaking scale M S . This signals that supersymmetry may be broken at high scale according to the cutoff leaving the naturalness issue aside. We suggest that relaxed supergravity can be a universal framework for building supergravity models of various phenomenologies under broken SUSY from particle physics to cosmology.

Complex Linear Multiplets and Local Supersymmetry Breaking

“…In a similar vein (as we will show in section 3) there has also been a study on new types of Fayet-Iliopoulos terms that lead to a breaking of supersymmetry without requiring the gauging of the R-symmetry [19][20][21][22][23]. The self-consistency of such terms, from the effective field theory perspective, has been scrutinized in [24,25], and possible alternatives have been also studied in [26][27][28] which relax some properties of supersymmetric scalar potentials. In addition, there exist modified (nilpotent or not) complex linear multiplets which can serve as the goldstino superfield [29,30], however in those cases the auxiliary fields do not necessarily have a VEV.…”