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T parity and the littlest Higgs

Ian Low
- 03 Dec 2004 - 
- Vol. 2004, Iss: 10, pp 067-067
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TLDR
In this paper, T-parity invariant extensions of the littlest Higgs model were constructed, in which only linear representations of the full symmetry group are employed, without recourse to the non-linear representations introduced by Coleman, Callan, Wess, and Zumino (CCWZ).
Abstract
We construct T-parity invariant extensions of the littlest Higgs model, in which only linear representations of the full symmetry group are employed, without recourse to the non-linear representations introduced by Coleman, Callan, Wess, and Zumino (CCWZ). These models are based on the symmetry breaking pattern SU(5)l × Hr/SO(5), where Hr can be SO(5) or other larger symmetry groups. The structure of the models in the SU(5)l sector is identical to the littlest Higgs model based on SU(5)/SO(5). Since the full symmetry group is realized linearly, these models can be thought of as possible UV extensions of the T-invariant model using non-linear representations via CCWZ, with whom they share similar low energy phenomenology. We also comment on how to avoid constraints from four-fermion operators on T-invariant models with or without CCWZ construction. The electroweak data therefore place a very weak bound on the symmetry breaking scale, f ≥ 450 GeV.

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TL;DR: In this article, the general structure of phenomenological Lagrangian theories is investigated, and the possible transformation laws of the phenomenological fields under a group are discussed, which is equivalent to finding all (nonlinear) realizations of a (compact, connected, semisimpleasure) Lie group which become linear when restricted to a given subgroup.
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TL;DR: In this paper, the general method for constructing invariant phenomenological Lagrangians is described, where the fields are assumed to transform according to (nonlinear) realizations of an internal symmetry group, given in standard form.
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Anthropic bound on the cosmological constant

TL;DR: It is argued here that in universes that do not recollapse, the only bound on the cosmological constantlambda is that it should not be so large as to prevent the formation of gravitationally bound states, and it turns out that the bound is quite large.
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Electroweak symmetry breaking from dimensional deconstruction

TL;DR: In this paper, a new class of four-dimensional theories for natural electroweak symmetry breaking, relying neither on supersymmetry nor on strong dynamics at the TeV scale, was proposed.
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