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A Composite Little Higgs Model

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Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
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Emanuel Katz, Jaeyong Lee, Ann E. Nelson, Devin G. E. Walker

High Energy Physics - Phenomenology · Submitted 20 Dec 2003

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim We describe a natural UV complete theory with a composite little Higgs.

how it is stated · asserted 1.00 read the record →

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arXiv IDhep-ph/0312287 (version 2)
Pith IDWCNJWC5K, Pith's permanent record of this paper and its review
CitationAnn E. Nelson, Devin G. E. Walker, Emanuel Katz, Jaeyong Lee. "A Composite Little Higgs Model." arXiv:hep-ph/0312287 (2003). https://pith.science/paper/WCNJWC5K
Claim paper

The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 7,524 input tokens, $0.0003 reported.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.11 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.39 · compares with prior results 0.18 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; .

We describe a natural UV complete theory with a composite little Higgs. Below a TeV we have the minimal Standard Model with a light Higgs, and an extra neutral scalar. At the TeV scale there are additional scalars, gauge bosons, and vector-like charge 2/3 quarks, whose couplings to the Higgs greatly reduce the UV sensitivity of the Higgs potential. Stabilization of the Higgs mass squared parameter, without finetuning, occurs due to a softly broken shift symmetry--the Higgs is a pseudo Nambu-Goldstone boson. Above the 10 TeV scale the theory has new strongly coupled interactions. A perturbatively renormalizable UV completion, with softly broken supersymmetry at 10 TeV is explicitly worked out. Our theory contains new particles which are odd under an exact "dark matter parity", (-1)^{(2S+3B+L)}. We argue that such a parity is likely to be a feature of many theories of new TeV scale physics. The lightest parity odd particle, or "LPOP", is most likely a neutral fermion, and may make a good dark matter candidate, with similar experimental signatures to the neutralino of the MSSM. We give a general effective field theory analysis of the calculation of corrections to precision electroweak observables.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 We describe a natural UV complete theory with a composite little Higgs. contribution 1.00 0.89 0.36 asserted 1.00
s1 Below a TeV we have the minimal Standard Model with a light Higgs, and an extra neutral scalar. result 0.54 0.49 0.09 asserted 1.00
s2 At the TeV scale there are additional scalars, gauge bosons, and vector-like charge 2/3 quarks, whose couplings to the Higgs greatly reduce the UV sensitivity of the Higgs potential. contribution 0.65 0.55 0.14 asserted 1.00
s3 Stabilization of the Higgs mass squared parameter, without finetuning, occurs due to a softly broken shift symmetry--the Higgs is a pseudo Nambu-Goldstone boson. result 0.54 0.63 0.23 asserted 1.00
s4 Above the 10 TeV scale the theory has new strongly coupled interactions. contribution 0.61 0.50 0.05 asserted 1.00
s5 A perturbatively renormalizable UV completion, with softly broken supersymmetry at 10 TeV is explicitly worked out. contribution 0.92 0.93 0.11 asserted 1.00
s6 Our theory contains new particles which are odd under an exact "dark matter parity", (-1)^{(2S+3B+L)}. result 0.62 0.80 0.10 asserted 1.00
s7 We argue that such a parity is likely to be a feature of many theories of new TeV scale physics. interpretation 1.00 0.36 0.10 hedged possibility 1.00
s8 The lightest parity odd particle, or "LPOP", is most likely a neutral fermion, and may make a good dark matter candidate, with similar experimental signatures to the neutralino of the MSSM. interpretation 0.92 0.50 0.14 hedged possibility 1.00
s9 We give a general effective field theory analysis of the calculation of corrections to precision electroweak observables. contribution 0.81 0.84 0.05 asserted 0.97

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.73.

What was examined, and what was not

sources read
  • arXiv listing abstract v2
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

We describe a natural UV complete theory with a composite little Higgs. Below a TeV we have the minimal Standard Model with a light Higgs, and an extra neutral scalar. At the TeV scale there are additional scalars, gauge bosons, and vector-like charge 2/3 quarks, whose couplings to the Higgs greatly reduce the UV sensitivity of the Higgs potential. Stabilization of the Higgs mass squared parameter, without finetuning, occurs due to a softly broken shift symmetry--the Higgs is a pseudo Nambu-Goldstone boson. Above the 10 TeV scale the theory has new strongly coupled interactions. A perturbatively renormalizable UV completion, with softly broken supersymmetry at 10 TeV is explicitly worked out. Our theory contains new particles which are odd under an exact "dark matter parity", (-1)^{(2S+3B+L)}. We argue that such a parity is likely to be a feature of many theories of new TeV scale physics. The lightest parity odd particle, or "LPOP", is most likely a neutral fermion, and may make a good dark matter candidate, with similar experimental signatures to the neutralino of the MSSM. We give a general effective field theory analysis of the calculation of corrections to precision electroweak observables.

Human review

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References
How the literature uses it

21 arXiv papers cite this in 36 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 24 sentences without a confident label

Cites it as background 12 papers

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