Published September 1, 2007 | Version v1
Journal article

Nonzero trilinear parameter in the minimal supergravity model: Dark matter and collider signals at the Fermilab Tevatron and CERN LHC

  • 1. Department of Theoretical Physics, Indian Association for the Cultivation of Science, Raja S.C. Mullick Road, Kolkata 700 032 (India)
  • 2. Department of Physics, Jadavpur University, Jadavpur, Kolkata 700 032 (India)

Description

Phenomenologically viable and interesting regions of parameter space in the minimal supergravity (mSUGRA) model with small m0 and small m1/2 consistent with the WMAP data on dark matter relic density and the bound on the mass of the lightest Higgs scalar mh>114 GeV from the Linear Electron Positron Collider open up if the rather ad hoc assumption A0=0, where A0 is the common trilinear soft breaking parameter, employed in most of the existing analyses is relaxed. Since this region corresponds to relatively light squarks and gluinos which are likely to be probed extensively in the very early stages of the LHC experiments, the consequences of moderate or large negative values of A0 are examined in detail. We find that in this region several processes including lightest supersymmetric particle (LSP) pair annihilation, LSP-lighter tau slepton (τ-tilde1) coannihilation and LSP--lighter top squark (t-tilde1) coannihilation contribute to the observed dark matter relic density. The possibility that a t-tilde1 that can participate in coannihilation with the lightest neutralino to satisfy the WMAP bound on relic density and at the same time be observed at the current experiments at the Tevatron is wide open. At the LHC a large number of squark-gluino events lead to a very distinctive semi-inclusive signature τ±+Xτ (anything without a tau lepton) with a characteristic size much larger than e±+Xe or μ±+Xμ events

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
76
Journal Issue
5
Journal Page Range
p. 055008-055008.12
ISSN
0556-2821
CODEN
PRVDAQ

Optional Information

Notes
(c) 2007 The American Physical Society