Published January 1, 1994 | Version v1
Journal article

Simplest, string-derivable, supergravity model and its experimental predictions

  • 1. Astroparticle Physics Group, Houston Advanced Research Center (HARC), The Woodlands, Texas 77381 (United States)
  • 2. Center for Theoretical Physics, Department of Physics, Texas A ampersand M University, College Station, Texas 77843-4242 (United States)
  • 3. CERN Theory Division, 1211 Geneva 23 (Switzerland)
  • 4. CERN, Geneva (Switzerland)

Description

We present the simplest, string-derivable, supergravity model and discuss its experimental consequences. This model is a new string-inspired flipped SU(5) which unifies at the string scale MU=1018 GeV due to the introduction of an additional pair of 10,1 bar 0 flipped SU(5) representations which contain new intermediate scale ''gap'' particles. We study various model-building issues which should be addressed in string-derived incarnations of this model. We focus our study on the no-scale supergravity mechanism and explore thoroughly the three-dimensional parameter space of the model (mg,mt,tanβ), thus obtaining several simple relationships among the particle masses, such as mq∼mg, meL∼mnu∼0.30mg, meR∼0.18mg, and mχ20∼2mχ10∼mχ1±. In a strict interpretation of the no-scale supergravity scenario we solve for tanβ as a function of mt and mg, and show that mt determines not only the sign of the Higgs mixing parameter μ but also whether the lightest Higgs boson mass is above or below 100 GeV. We also find that throughout the parameter space the neutralino relic abundance is within observational bounds (Ωχh02 approx-lt 0.25) and may account for a significant portion of the dark matter in the Universe

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
49
Journal Issue
1
Journal Page Range
p. 343-354.
ISSN
0556-2821
CODEN
PRVDAQ