On low-energy supersymmetry breaking through gaugino masses in superstring-inspired models

1987 ◽  
Vol 186 (3-4) ◽  
pp. 356-360 ◽  
Author(s):  
G.D. Coughlan ◽  
G. Germán
1987 ◽  
Vol 02 (01) ◽  
pp. 49-55 ◽  
Author(s):  
PARTHASARATHI MAJUMDAR

The gravitino contribution to the one loop gaugino self energy in low energy N=1 supergravity models derived from superstrings is considered. This contribution is shown to vanish when a supersymmetric regularization procedure is used. An identical conclusion is seen to hold for the contribution of the fermionic component of the gauge singlet chiral supermultiplet that arises out of gaugino condensation in the Hidden (‘shadow’) sector. Implications for supersymmetry breaking in the observable sector of superstring theories are briefly discussed.


2006 ◽  
Vol 2006 (04) ◽  
pp. 040-040 ◽  
Author(s):  
Benjamin C Allanach ◽  
Fernando Quevedo ◽  
Kerim Suruliz

2021 ◽  
Vol 2021 (8) ◽  
Author(s):  
Anthony Ashmore ◽  
Sebastian Dumitru ◽  
Burt A. Ovrut

Abstract The strongly coupled heterotic M-theory vacuum for both the observable and hidden sectors of the B − L MSSM theory is reviewed, including a discussion of the “bundle” constraints that both the observable sector SU(4) vector bundle and the hidden sector bundle induced from a single line bundle must satisfy. Gaugino condensation is then introduced within this context, and the hidden sector bundles that exhibit gaugino condensation are presented. The condensation scale is computed, singling out one line bundle whose associated condensation scale is low enough to be compatible with the energy scales available at the LHC. The corresponding region of Kähler moduli space where all bundle constraints are satisfied is presented. The generic form of the moduli dependent F-terms due to a gaugino superpotential — which spontaneously break N = 1 supersymmetry in this sector — is presented and then given explicitly for the unique line bundle associated with the low condensation scale. The moduli-dependent coefficients for each of the gaugino and scalar field soft supersymmetry breaking terms are computed leading to a low-energy effective Lagrangian for the observable sector matter fields. We then show that at a large number of points in Kähler moduli space that satisfy all “bundle” constraints, these coefficients are initial conditions for the renormalization group equations which, at low energy, lead to completely realistic physics satisfying all phenomenological constraints. Finally, we show that a substantial number of these initial points also satisfy a final constraint arising from the quadratic Higgs-Higgs conjugate soft supersymmetry breaking term.


2002 ◽  
Vol 11 (08) ◽  
pp. 1159-1169 ◽  
Author(s):  
I. L. SHAPIRO

The stable version of the anomaly-induced inflation does not need a fine tuning to induce sufficient expansion of the Universe. The non-stable version (Starobinsky model) provides the graceful exit to the FRW phase. Here, we indicate the possibility of the inflation which is stable at the beginning and unstable at the end. The effect is due to the soft supersymmetry breaking and the decoupling of the massive sparticles at low energy.


2018 ◽  
Vol 98 (11) ◽  
Author(s):  
Anson Hook ◽  
Robert McGehee ◽  
Hitoshi Murayama

2018 ◽  
Vol 182 ◽  
pp. 02005
Author(s):  
I. Antoniadis

I describe the phenomenology of a model of supersymmetry breaking in the presence of a tiny (tuneable) positive cosmological constant. It utilises a single chiral multiplet with a gauged shift symmetry, that can be identified with the string dilaton (or an appropriate compactification modulus). The model is coupled to the MSSM, leading to calculable soft supersymmetry breaking masses and a distinct low energy phenomenology that allows to differentiate it from other models of supersymmetry breaking and mediation mechanisms. We also study the question if this model can lead to inflation by identifying the dilaton with the inflaton. We find that this is possible if the Kähler potential is modified by a term that has the form of NS5-brane instantons, leading to an appropriate inflationary plateau around the maximum of the scalar potential, depending on two extra parameters.


1996 ◽  
Vol 54 (5) ◽  
pp. 3283-3288 ◽  
Author(s):  
Savas Dimopoulos ◽  
Scott Thomas ◽  
James D. Wells

2005 ◽  
Vol 20 (18) ◽  
pp. 4241-4257 ◽  
Author(s):  
B. ANANTHANARAYAN ◽  
P. N. PANDITA

We consider supersymmetric SO(10) grand unification where the unified gauge group can break to the Standard Model gauge group through different chains. The breaking of SO(10) necessarily involves the reduction of the rank, and consequent generation of nonuniversal supersymmetry breaking scalar mass terms. We derive squark and slepton mass relations, taking into account these nonuniversal contributions to the sfermion masses, which can help distinguish between the different chains through which the SO(10) gauge group breaks to the Standard Model gauge group. We then study some implications of these nonuniversal supersymmetry breaking scalar masses for the low energy phenomenology.


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