Abstract

A novel realization of the gravity-mediated SUSY breaking is presented taking into account a continuous global R symmetry. Consistently with it, we employ a linear superpotential for the hidden sector superfield and a Kaehler potential parameterizing the SU(1,1)/U(1) Kaehler manifold with constant curvature -1/2. The classical vacuum energy vanishes without unnatural fine tuning and non-vanishing soft SUSY-breaking parameters, of the order of the gravitino mass, arise. A solution to the mu problem of MSSM may be also achieved by conveniently applying the Giudice-Masiero mechanism. The potentially troublesome R axion may acquire acceptably large mass by explicitly breaking the R symmetry in the Kaehler potential through a quartic term which does not affect, though, the achievements above.

Highlights

  • Still undiscovered, supersymmetry (SUSY) remains one of the most plausible, well-motivated, and natural candidates for the evolution of particle physics beyond the Standard Model (SM)

  • According to an elegant and extensively adopted paradigm, SUSY is spontaneously broken by the vacuum expectation values (VEVs) of a set of chiral fields which form a “hidden sector” [1] connecting with the observable sector mostly through gravitational-strength interactions, including the effects of supergravity (SUGRA)

  • One of the key ingredients for the successful implementation of this scenario is the determination of a realistic vacuum for the relevant SUGRA potential with a naturally vanishing or, at least, tunably small cosmological constant

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Summary

INTRODUCTION

Supersymmetry (SUSY) remains one of the most plausible, well-motivated, and natural candidates for the evolution of particle physics beyond the Standard Model (SM). Contrary to that case [13], the gravitino, G , mass is clearly determined at the tree level and the soft SUSY-breaking (SSB) parameters [14] can readily acquire adjustable, nonzero values of the order of Gmass. We exemplify these effects, linking the hidden sector to a generic SUSY model and the minimal supersymmetric SM (MSSM). A spontaneously broken continuous and global R symmetry implies an (pseudo) Nambu-Goldstone boson, the R axion [6,16]—as in the case of Peccei-Quinn symmetry [17]—which is cosmologically dangerous To avoid this effect, we introduce a quartic term, inspired by Ref. Stated, we use units where the reduced Planck mass mP 1⁄4 2.433 × 1018 GeV is taken to be unity and charge conjugation is denoted by a bar

SUGRA FORMALISM
HIDDEN SECTOR
Model setup
Totally R-symmetric case
Including the R-symmetry-breaking term
OBSERVABLE SECTOR
Generic model
Scalar sector and Generation of the μ-term
Gaugino sector
Caa hðFZ a
CONCLUSIONS AND PERSPECTIVES
Half-plane formulation
Hidden-sector spectrum
Soft SUSY-breaking parameters
Full Text
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