Searching for dark matter in unification models: A hint from indirect sensitivities towards future signals in direct detection and B-decays

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

A comparison is made between accelerator and direct detection constraints in constrained versions of the minimal supersymmetric standard model. Models considered are based on mSUGRA, where scalar and gaugino masses are unified at the GUT scale. In addition, the mSUGRA relation between the (unified) A and B parameters is assumed, as is the relation between m0 and the gravitino mass. Also considered are models where the latter two conditions are dropped (the CMSSM), and a less constrained version where the Higgs soft masses are not unified at the GUT scale (the NUHM).

Original languageEnglish (US)
Title of host publicationTHE DARK SIDE OF THE UNIVERSE
Subtitle of host publication2nd International Conference on The Dark Side of the Universe DSU 2006
Pages34-45
Number of pages12
DOIs
StatePublished - 2006
EventTHE DARK SIDE OF THE UNIVERSE: 2nd International Conference on The Dark Side of the Universe DSU 2006 - Madrid, Spain
Duration: Jun 20 2006Jun 24 2006

Publication series

NameAIP Conference Proceedings
Volume878
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherTHE DARK SIDE OF THE UNIVERSE: 2nd International Conference on The Dark Side of the Universe DSU 2006
Country/TerritorySpain
CityMadrid
Period6/20/066/24/06

Keywords

  • Dark matter
  • Supersymmetry

Fingerprint

Dive into the research topics of 'Searching for dark matter in unification models: A hint from indirect sensitivities towards future signals in direct detection and B-decays'. Together they form a unique fingerprint.

Cite this