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Non-universalities in pure gravity mediation

  • Jason L. EvansEmail author
  • Masahiro Ibe
  • Keith A. Olive
  • Tsutomu T. Yanagida
Regular Article - Theoretical Physics

Abstract

The simplest model of pure gravity mediation contains only two free parameters: the gravitino mass and tanβ. Scalar masses are universal at some high energy renormalization scale and gaugino masses are determined through anomalies and depend on the gravitino mass and the gauge couplings. This theory requires a relatively large gravitino mass (m 3/2≳300 TeV) and a limited range in tanβ≃1.7–2.5. Here we generalize the theory to allow for non-universality in the Higgs soft masses. This introduces zero, one or two new free parameters associated with Higgs soft masses. This generalization allows us to greatly increase the allowed range in tanβ and it allows one to find viable solutions with lower m 3/2. The latter is important if we hope to find a low energy signal from gluinos. Some special cases of these non-universalities are suggestive of Higgs bosons as Nambu–Goldstone bosons or a partial no-scale structure for the Higgs doublets. Thus, we probe signatures at the weak scale and structures at the GUT and/or Planck scale.

Keywords

Higgs Boson Light Supersymmetric Particle Higgs Doublet Goldstone Boson Soft Mass 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Notes

Acknowledgements

The work of J.E. and K.A.O. was supported in part by DOE grant DE–FG02–94ER–40823 at the University of Minnesota. This work is also supported by Grant-in-Aid for Scientific research from the Ministry of Education, Science, Sports, and Culture (MEXT), Japan, No. 22244021 (T.T.Y.), No. 24740151 (M.I.), and also by the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan.

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Copyright information

© Springer-Verlag Berlin Heidelberg and Società Italiana di Fisica 2013

Authors and Affiliations

  • Jason L. Evans
    • 1
    Email author
  • Masahiro Ibe
    • 2
    • 3
  • Keith A. Olive
    • 1
  • Tsutomu T. Yanagida
    • 3
  1. 1.William I. Fine Theoretical Physics Institute, School of Physics and AstronomyUniversity of MinnesotaMinneapolisUSA
  2. 2.ICRRUniversity of TokyoKashiwaJapan
  3. 3.Kavli IPMU (WPI), TODIASUniversity of TokyoKashiwaJapan

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