Higher-Derivative Gravitation and a New Mechanism for Supersymmetry Breaking in Four-Dimensions

TL;DR

This paper explores higher-derivative gravity theories in four dimensions, revealing their degrees of freedom, coupling mechanisms, and demonstrating that certain models can spontaneously break supersymmetry while maintaining stable vacua with zero cosmological constant.

Contribution

It introduces a complete non-linear sigma model for higher-derivative gravitational degrees of freedom and shows how these theories can spontaneously break supersymmetry with stable vacua.

Findings

Higher-derivative terms lead to additional degrees of freedom.

Certain supergravity models exhibit stable vacua with broken supersymmetry.

Higher-derivative supergravity is equivalent to coupled chiral supermultiplets.

Abstract

A discussion of the number of degrees of freedom, and their dynamical properties, in higher derivative gravitational theories is presented. The complete non-linear sigma model for these degrees of freedom is exhibited using the method of auxiliary fields. As a by-product we present a consistent non-linear coupling of a spin-2 tensor to gravitation. It is shown that non-vanishing $(C_{\mu\nu\alpha\beta})^2$ terms arise in $N=1$, $D=4$ superstring Lagrangians due to one-loop radiative corrections with light field internal lines. We discuss the general form of quadratic $(1,1)$ supergravity in two dimensions, and show that this theory is equivalent to two scalar supermultiplets coupled to the usual Einstein supergravity. It is demonstrated that the theory possesses stable vacua with vanishing cosmological constant which spontaneously break supersymmetry. We then generalize this result to $N=1$ supergravity in four dimensions. Specifically, we demonstrate that a class of higher derivative supergravity theories is equivalent to two chiral supermultiplets coupled in a specific way to Einstein supergravity. These theories are shown to possess stable vacuum states with vanishing cosmological constant which spontaneously break the $N=1$ supersymmetry.