Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Sneutrino NLSP in the {nu}CMSSM

Journal Article · · Physical Review. D, Particles Fields
 [1];  [2];  [3]
  1. Michigan Center for Theoretical Physics, University of Michigan, Ann Arbor, Michigan 48109 (United States)
  2. William I. Fine Theoretical Physics Institute, University of Minnesota, Minneapolis, Minnesota 55455 (United States)
  3. The Abdus Salam International Center for Theoretical Physics, 34014 Trieste (Italy)

We extend the constrained minimal supersymmetric model (CMSSM) by adding a right-handed neutrino superfield ({nu}CMSSM) which decouples close to the GUT scale. We study the effects of a right-handed neutrino on the low energy spectrum and focus on the predictions for dark matter properties. We pay particular attention to the realization of the light (left-handed) sneutrino which can be the next-to-lightest supersymmetric particle (NLSP) with either the neutralino or gravitino as the lightest supersymmetric particle (LSP). Notably, for the case of a neutralino LSP with a sneutrino NLSP, there are new 'sneutrino coannihilation regions' which yield the desired thermal neutralino relic density determined by WMAP.

OSTI ID:
21260112
Journal Information:
Physical Review. D, Particles Fields, Journal Name: Physical Review. D, Particles Fields Journal Issue: 5 Vol. 79; ISSN PRVDAQ; ISSN 0556-2821
Country of Publication:
United States
Language:
English

Similar Records

Reconstruction of the left-chiral tau sneutrino in supersymmetry with a right sneutrino as the lightest supersymmetric particle
Journal Article · Fri Oct 01 00:00:00 EDT 2010 · Physical Review. D, Particles Fields · OSTI ID:21432329

Heavy right-handed neutrinos and dark matter in the {nu}CMSSM
Journal Article · Sun Nov 01 00:00:00 EDT 2009 · Physical Review. D, Particles Fields · OSTI ID:21325500

Cosmological constraints on the gravitino LSP scenario with a sneutrino NLSP
Journal Article · Sun Jan 14 23:00:00 EST 2007 · Physical Review. D, Particles Fields · OSTI ID:21010924