scholarly journals Gauge mediation with D terms

2011 ◽  
Vol 2011 (5) ◽  
Author(s):  
Linda M. Carpenter
Keyword(s):  
Gauge Mediation

scholarly journals Gauge Mediation Simplified

2007 ◽  
Vol 98 (15) ◽  
Author(s):  
Hitoshi Murayama ◽  
Yasunori Nomura
Keyword(s):  
Gauge Mediation

scholarly journals Study of the gauge mediation signal with nonpointing photons at the CERN LHC

2004 ◽  
Vol 69 (3) ◽  
Author(s):  
Kiyotomo Kawagoe ◽  
Tomio Kobayashi ◽  
Mihoko M. Nojiri ◽  
Atsuhiko Ochi
Keyword(s):  
Gauge Mediation

scholarly journals Gauge-mediation model of dynamical SUSY breaking with a wide range of the gravitino mass

1999 ◽  
Vol 452 (3-4) ◽  
pp. 274-278 ◽  
Author(s):  
K.-I. Izawa ◽  
Yasunori Nomura ◽  
T. Yanagida
Keyword(s):  
Susy Breaking ◽  
Gauge Mediation ◽  
Mediation Model ◽  
Gravitino Mass ◽  
Wide Range

scholarly journals The light stop scenario from gauge mediation

2012 ◽  
Vol 2012 (4) ◽  
Author(s):  
Antonio Delgado ◽  
Germano Nardini ◽  
Mariano Quirós
Keyword(s):  
Gauge Mediation ◽  
Light Stop

scholarly journals Low-scale gauge mediation after LHC Run 2

2018 ◽  
Vol 784 ◽  
pp. 237-247 ◽  
Author(s):  
Xiaochuan Lu ◽  
Satoshi Shirai
Keyword(s):  
Gauge Mediation

scholarly journals Cosmology of supersymmetric models with low-energy gauge mediation

1997 ◽  
Vol 56 (2) ◽  
pp. 1281-1299 ◽  
Author(s):  
André de Gouve⁁a ◽  
Takeo Moroi ◽  
Hitoshi Murayama
Keyword(s):  
Low Energy ◽  
Gauge Mediation ◽  
Supersymmetric Models

scholarly journals Low fine-tuning in Yukawa-deflected gauge mediation

2017 ◽  
Vol 95 (9) ◽  
Author(s):  
Waqas Ahmed ◽  
Lorenzo Calibbi ◽  
Tianjun Li ◽  
Azar Mustafayev ◽  
Shabbar Raza
Keyword(s):  
Fine Tuning ◽  
Gauge Mediation

scholarly journals Phenomenology of Minimal Unified Tree Level Gauge Mediation at the LHC

2013 ◽  
Vol 2013 (7) ◽  
Author(s):  
Maurizio Monaco ◽  
Maurizio Pierini ◽  
Andrea Romanino ◽  
Martin Spinrath
Keyword(s):  
Level Gauge ◽  
Tree Level ◽  
Gauge Mediation

scholarly journals Focus point gauge mediation with incomplete adjoint messengers and gauge coupling unification

2015 ◽  
Vol 749 ◽  
pp. 82-87 ◽  
Author(s):  
Gautam Bhattacharyya ◽  
Tsutomu T. Yanagida ◽  
Norimi Yokozaki
Keyword(s):  
Gauge Coupling ◽  
Gauge Mediation ◽  
Focus Point

WHY IS THE HIDDEN SECTOR INVISIBLE?

2000 ◽  
Vol 15 (35) ◽  
pp. 2131-2137 ◽  
Author(s):  
M. D. POLLOCK
Keyword(s):  
Degrees Of Freedom ◽  
Coupling Parameter ◽  
Vacuum State ◽  
Fine Tuning ◽  
Gauge Mediation ◽  
Superstring Theory ◽  
Thermodynamical Equilibrium ◽  
Hidden Sector ◽  
Axion Field ◽  
Model Independent

The hidden sector of the E8×E′8 heterotic superstring theory of Gross et al. can in principle contain additional "shadow" matter, interacting only gravitationally with the real world in which we live. The SU (3)′ C × SU (2)′ L × U (1)′ Y shadow configuration symmetric to the standard model has been ruled out by Kolb et al. from nucleosynthesis arguments, combined with the existence of three light neutrinos. In the absence of inflation and of entropy enhancement by the out-of-equilibrium decay of an unstable particle, the same exclusion applies to the unbroken E′8 hidden gauge group, assuming thermodynamical equilibrium with the observable sector E6 group, and consequently all breaking chains E′8→ G1×G2×⋯, since they can only reduce the effective number of four-dimensional degrees of freedom g eff . The hidden sector would then appear to be in its vacuum state, which implies the absence of all condensates as well, if their potentials are positive semi-definite. In this case, and if there is no anomalous U(1) symmetry in the observable sector, the QCD axion is the model-independent axion, whose decay constant [Formula: see text] (where [Formula: see text] is the strong-interaction coupling parameter) requires a fine-tuning of the initial value of this axion field to ai/fa≲3×10-3, in order not to overclose the Universe today, supersymmetry being broken by gauge mediation. Vice versa, if ai/fa~1, then hidden-sector gaugino condensation is necessary for there to be a sufficiently massive gravitino, whose decay can increase the entropy. Astronomical microlensing observations may help to discriminate between these two cases.

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