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Zeroing in on Supersymmetric Radiation Amplitude Zeros

High Energy Physics - Phenomenology · Submitted 18 Oct 2011

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

The authors' main claim We test this technique on a previously generated model sample of the 19 dimensional parameter space of the phenomenological MSSM, and find that it is effective in determining the wino content of the neutralino.

how it is stated · asserted 1.00 read the record →

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arXiv ID1110.4144 (version 1)
Pith IDABFRXB47, Pith's permanent record of this paper and its review
CitationAhmed Ismail, JoAnne L. Hewett, Thomas G. Rizzo. "Zeroing in on Supersymmetric Radiation Amplitude Zeros." arXiv:1110.4144 (2011). https://pith.science/paper/ABFRXB47
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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, 4,417 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.06 · states limitation 0.20 · human participants 0.01 · controlled comparison 0.94 · randomized assignment 0.01 · states quantitative result 0.07 · compares with prior results 0.51 · mentions code or data availability 0.03.

The abstract, sentence by sentence

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

Radiation amplitude zeros have long been used to test the Standard Model. Here, we consider the supersymmetric radiation amplitude zero in chargino-neutralino associated production, which can be observed at the luminosity upgraded LHC. Such an amplitude zero only occurs if the neutralino has a large wino fraction and hence this observable can be used to determine the neutralino eigenstate content. We find that this observable can be measured by comparing the p_T spectrum of the softest lepton in the trilepton $\chi_1^\pm \chi_2^0$ decay channel to that of a control process such as $\chi_1^+ \chi_1^-$ or $\chi_2^0 \chi_2^0$. We test this technique on a previously generated model sample of the 19 dimensional parameter space of the phenomenological MSSM, and find that it is effective in determining the wino content of the neutralino.

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 Radiation amplitude zeros have long been used to test the Standard Model. background 1.00 0.04 0.02 asserted 1.00
s1 Here, we consider the supersymmetric radiation amplitude zero in chargino-neutralino associated production, which can be observed at the luminosity upgraded LHC. contribution 1.00 0.70 0.06 hedged possibility 0.64
s2 Such an amplitude zero only occurs if the neutralino has a large wino fraction and hence this observable can be used to determine the neutralino eigenstate content. interpretation 0.68 0.26 0.38 asserted 0.99
s3 We find that this observable can be measured by comparing the p_T spectrum of the softest lepton in the trilepton $\chi_1^\pm \chi_2^0$ decay channel to that of a control process such as $\chi_1^+ \chi_1^-$ or $\chi_2^0 \chi_2^0$. method 0.99 0.89 0.12 asserted 0.95
s4 We test this technique on a previously generated model sample of the 19 dimensional parameter space of the phenomenological MSSM, and find that it is effective in determining the wino content of the neutralino. result 0.86 0.96 0.61 asserted 1.00

What kind of paper the classifier reports this is: method or tool 0.93 · evidence from simulation or computation 0.74.

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not examined
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  • figures and tables
  • references and citing sentences
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  • T body sentences
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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

Radiation amplitude zeros have long been used to test the Standard Model. Here, we consider the supersymmetric radiation amplitude zero in chargino-neutralino associated production, which can be observed at the luminosity upgraded LHC. Such an amplitude zero only occurs if the neutralino has a large wino fraction and hence this observable can be used to determine the neutralino eigenstate content. We find that this observable can be measured by comparing the p_T spectrum of the softest lepton in the trilepton $\chi_1^\pm \chi_2^0$ decay channel to that of a control process such as $\chi_1^+ \chi_1^-$ or $\chi_2^0 \chi_2^0$. We test this technique on a previously generated model sample of the 19 dimensional parameter space of the phenomenological MSSM, and find that it is effective in determining the wino content of the neutralino.

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1 arXiv paper cite this in 1 sentence

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

Cites it as background 1 paper
  • For instance, one has the SM process $ud̅ →γW^+$ [ref] , the high $p_T$ chargino-neutralino production of SUSY [ref] , and the lepto-quark process [ref] .

    Dips at Colliders · Introduction · 0.91

What it cites · 12 sentences without a confident label

Uses data or values from 1 paper
  • To evaluate the potential of our technique, we make use of a previous scan [ref] over the phenomenological MSSM (pMSSM) parameter space and examine the signature of amplitude zeros in a sample of supersymmetric models.

    Supersymmetry Without Prejudice · Introduction · 0.95

Cites as background 2 papers

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