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Direct-Transmission Models of Dynamical Supersymmetry Breaking

High Energy Physics - Phenomenology · Submitted 5 May 1997

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

The authors' main claim We obtain a natural model with the gravitino mass $m_{3/2}$ smaller than 1 keV as required from the standard cosmology.

how it is stated · asserted 1.00 read the record →

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arXiv IDhep-ph/9705228 (version 1)
Pith IDNJV53MS4, Pith's permanent record of this paper and its review
CitationK.-I. Izawa, K. Tobe, T. Yanagida, Y. Nomura. "Direct-Transmission Models of Dynamical Supersymmetry Breaking." arXiv:hep-ph/9705228 (1997). https://pith.science/paper/NJV53MS4
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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.

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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,868 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.38 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.98 · compares with prior results 0.06 · mentions code or data availability 0.01.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

We systematically construct gauge-mediated supersymmetry(SUSY)-breaking models with direct transmission of SUSY-breaking effects to the standard-model sector. We obtain a natural model with the gravitino mass $m_{3/2}$ smaller than 1 keV as required from the standard cosmology. If all Yukawa coupling constants are of order one,the SUSY-breaking scale $m_{SUSY}$ transmitted into the standard-model sector is given by $m_{SUSY} \simeq 0.1 \alpha_i/(4\pi) \Lambda$ where $\Lambda$ is the original dynamical SUSY-breaking scale. Imposing $m_{SUSY} \simeq (10^2-10^3)$ GeV, we get $\Lambda \simeq (10^5-10^6)$ GeV, which yields the gravitino mass $m_{3/2}\simeq (10^{-2}-1)$ keV.

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 systematically construct gauge-mediated supersymmetry(SUSY)-breaking models with direct transmission of SUSY-breaking effects to the standard-model sector. contribution 0.96 0.94 0.19 asserted 1.00
s1 We obtain a natural model with the gravitino mass $m_{3/2}$ smaller than 1 keV as required from the standard cosmology. result 0.95 0.93 0.21 asserted 1.00
s2 If all Yukawa coupling constants are of order one,the SUSY-breaking scale $m_{SUSY}$ transmitted into the standard-model sector is given by $m_{SUSY} \simeq 0.1 \alpha_i/(4\pi) \Lambda$ where $\Lambda$ is the original dynamical SUSY-breaking scale. result 1.00 0.81 0.29 asserted 0.96
s3 Imposing $m_{SUSY} \simeq (10^2-10^3)$ GeV, we get $\Lambda \simeq (10^5-10^6)$ GeV, which yields the gravitino mass $m_{3/2}\simeq (10^{-2}-1)$ keV. result 0.98 0.88 0.27 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.97.

What was examined, and what was not

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  • references and citing sentences
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  • C citations
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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 systematically construct gauge-mediated supersymmetry(SUSY)-breaking models with direct transmission of SUSY-breaking effects to the standard-model sector. We obtain a natural model with the gravitino mass $m_{3/2}$ smaller than 1 keV as required from the standard cosmology. If all Yukawa coupling constants are of order one,the SUSY-breaking scale $m_{SUSY}$ transmitted into the standard-model sector is given by $m_{SUSY} \simeq 0.1 \alpha_i/(4\pi) \Lambda$ where $\Lambda$ is the original dynamical SUSY-breaking scale. Imposing $m_{SUSY} \simeq (10^2-10^3)$ GeV, we get $\Lambda \simeq (10^5-10^6)$ GeV, which yields the gravitino mass $m_{3/2}\simeq (10^{-2}-1)$ keV.

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References
How the literature uses it

33 arXiv papers cite this in 49 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 · 36 sentences without a confident label

Builds on it 1 paper
Compares with it 1 paper
Cites it as background 10 papers
  • First, we review the model [ref] based on the IYIT model [ref] as a SUSY breaking sector.

    LHC Reach of Low Scale Gauge Mediation with Perturbatively Stable Vacuum · Model A (based on the IYIT model) · 0.82

  • This model is based on the recent development of metastable SUSY breaking in supersymmetric QCD (SQCD) started from the work of Intriligator, Seiberg and Shih (ISS) [ref] and is classified as so-called direct gauge mediation models [ref] where the flavor symmetries of a hidden SUSY breaking sector are weakly gauged and identified with the standard model gauge symmetries.

    Inflation in Gauge Mediation and Gravitino Dark Matter · Introduction · 0.80

  • We begin by considering a simple example of the messenger sector[Low energy description of direct GMSB models is often given by superpotentials of this type [ref] .]: [equation] Where $S$ is a supersymmetry breaking field and $ψ$, $ψ̅$ are messenger fields.

    Cascade supersymmetry breaking and low-scale gauge mediation · R-symmetry and the messenger sector · 0.86

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