z-logo
open-access-imgOpen Access
A composite little Higgs model
Author(s) -
Emanuel Katz,
Jae Yong Lee,
Ann E. Nelson,
Devin G. E. Walker
Publication year - 2005
Publication title -
journal of high energy physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.998
H-Index - 261
eISSN - 1126-6708
pISSN - 1029-8479
DOI - 10.1088/1126-6708/2005/10/088
Subject(s) - physics , particle physics , higgs boson , electroweak interaction , physics beyond the standard model , dark matter , neutralino , supersymmetry , standard model (mathematical formulation) , technicolor , effective field theory , higgs mechanism , higgs field , gauge boson , higgs sector , gauge theory , gauge (firearms) , archaeology , history
We describe a natural UV complete theory with a composite little Higgs. Belowa TeV we have the minimal Standard Model with a light Higgs, and an extraneutral scalar. At the TeV scale there are additional scalars, gauge bosons,and vector-like charge 2/3 quarks, whose couplings to the Higgs greatly reducethe UV sensitivity of the Higgs potential. Stabilization of the Higgs masssquared parameter, without finetuning, occurs due to a softly broken shiftsymmetry--the Higgs is a pseudo Nambu-Goldstone boson. Above the 10 TeV scalethe theory has new strongly coupled interactions. A perturbativelyrenormalizable UV completion, with softly broken supersymmetry at 10 TeV isexplicitly worked out. Our theory contains new particles which are odd under anexact "dark matter parity", (-1)^{(2S+3B+L)}. We argue that such a parity islikely to be a feature of many theories of new TeV scale physics. The lightestparity odd particle, or "LPOP", is most likely a neutral fermion, and may makea good dark matter candidate, with similar experimental signatures to theneutralino of the MSSM. We give a general effective field theory analysis ofthe calculation of corrections to precision electroweak observables.Comment: 28 page

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom