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A Heavy Gluino as the Lightest Supersymmetric Particle

High Energy Physics - Phenomenology · Submitted 13 Jun 1998

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

The authors' main claim We explore how the range of excluded gluino mass depends upon these ingredients, concluding that for non-extreme cases the range $3\gev\lsim\mgl\lsim 130-150\gev$ can be excluded at 95% CL based on currently available OPAL and CDF analyses.

how it is stated · asserted 0.95 read the record →

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arXiv IDhep-ph/9806361 (version 2)
Pith IDUSRHXOZP, Pith's permanent record of this paper and its review
CitationH. Baer, J.F. Gunion (U.C. Davis), K. Cheung. "A Heavy Gluino as the Lightest Supersymmetric Particle." arXiv:hep-ph/9806361 (1998). https://pith.science/paper/USRHXOZP
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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.

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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 7,903 input tokens, $0.0003 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.50 · human participants 0.01 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.99 · compares with prior results 0.54 · mentions code or data availability 0.01.

The abstract, sentence by sentence

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

We consider the possibility that the lightest supersymmetric particle is a heavy gluino. After discussing models in which this is the case, we demonstrate that the gluino-LSP could evade cosmological and other constraints by virtue of having a very small relic density. We then consider how neutral and charged hadrons containing a gluino will behave in a detector, demonstrating that there is generally substantial apparent missing momentum associated with a produced gluino-LSP. We next investigate limits on a (heavy) gluino-LSP deriving from LEP, LEP2 and RunI Tevatron experimental searches for excess events in the jets plus missing momentum channel and for stable heavily-ionizing charged particles. The range of gluino mass that can be excluded depends upon the path length of the gluino in the detector, the amount of energy it deposits in each hadronic collision, and the probability for the gluino to fragment to a pseudo-stable charged hadron after a given hadronic collision. We explore how the range of excluded gluino mass depends upon these ingredients, concluding that for non-extreme cases the range $3\gev\lsim\mgl\lsim 130-150\gev$ can be excluded at 95% CL based on currently available OPAL and CDF analyses. We find that RunII at the Tevatron can extend the excluded region (or discover the gluino) up to $\mgl\sim 160-180\gev$. For completeness, we also analyze the case where the gluino is the NLSP (as possible in gauge-mediated supersymmetry breaking) decaying via gluino -> g + gravitino. We find that the Tevatron RunI data excludes $\mgl\leq 240$ GeV. Finally, we discuss application of the procedures developed for the heavy gluino-LSP to searches for other stable strongly interacting particles, such as a stable heavy quark.

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 consider the possibility that the lightest supersymmetric particle is a heavy gluino. contribution 0.73 0.35 0.08 hedged possibility 0.90
s1 After discussing models in which this is the case, we demonstrate that the gluino-LSP could evade cosmological and other constraints by virtue of having a very small relic density. result 0.62 0.82 0.19 hedged possibility 0.58
s2 We then consider how neutral and charged hadrons containing a gluino will behave in a detector, demonstrating that there is generally substantial apparent missing momentum associated with a produced gluino-LSP. contribution 0.45 0.89 0.06 asserted 0.99
s3 We next investigate limits on a (heavy) gluino-LSP deriving from LEP, LEP2 and RunI Tevatron experimental searches for excess events in the jets plus missing momentum channel and for stable heavily-ionizing charged particles. method 0.58 0.80 0.04 asserted 0.90
s4 The range of gluino mass that can be excluded depends upon the path length of the gluino in the detector, the amount of energy it deposits in each hadronic collision, and the probability for the gluino to fragment to a pseudo-stable charged hadron after a given hadronic collision. method 0.77 0.45 0.05 asserted 0.99
s5 We explore how the range of excluded gluino mass depends upon these ingredients, concluding that for non-extreme cases the range $3\gev\lsim\mgl\lsim 130-150\gev$ can be excluded at 95% CL based on currently available OPAL and CDF analyses. result 1.00 0.89 0.46 asserted 0.95
s6 We find that RunII at the Tevatron can extend the excluded region (or discover the gluino) up to $\mgl\sim 160-180\gev$. result 0.94 0.88 0.15 asserted 0.83
s7 For completeness, we also analyze the case where the gluino is the NLSP (as possible in gauge-mediated supersymmetry breaking) decaying via gluino -> g + gravitino. contribution 0.97 0.67 0.02 hedged possibility 0.83
s8 We find that the Tevatron RunI data excludes $\mgl\leq 240$ GeV. result 1.00 0.87 0.10 asserted 1.00
s9 Finally, we discuss application of the procedures developed for the heavy gluino-LSP to searches for other stable strongly interacting particles, such as a stable heavy quark. contribution 0.63 0.70 0.04 asserted 0.64

What kind of paper the classifier reports this is: theoretical result 0.94 · evidence from analysis of existing data 0.97.

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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 consider the possibility that the lightest supersymmetric particle is a heavy gluino. After discussing models in which this is the case, we demonstrate that the gluino-LSP could evade cosmological and other constraints by virtue of having a very small relic density. We then consider how neutral and charged hadrons containing a gluino will behave in a detector, demonstrating that there is generally substantial apparent missing momentum associated with a produced gluino-LSP. We next investigate limits on a (heavy) gluino-LSP deriving from LEP, LEP2 and RunI Tevatron experimental searches for excess events in the jets plus missing momentum channel and for stable heavily-ionizing charged particles. The range of gluino mass that can be excluded depends upon the path length of the gluino in the detector, the amount of energy it deposits in each hadronic collision, and the probability for the gluino to fragment to a pseudo-stable charged hadron after a given hadronic collision. We explore how the range of excluded gluino mass depends upon these ingredients, concluding that for non-extreme cases the range $3\gev\lsim\mgl\lsim 130-150\gev$ can be excluded at 95% CL based on currently available OPAL and CDF analyses. We find that RunII at the Tevatron can extend the excluded region (or discover the gluino) up to $\mgl\sim 160-180\gev$. For completeness, we also analyze the case where the gluino is the NLSP (as possible in gauge-mediated supersymmetry breaking) decaying via gluino -> g + gravitino. We find that the Tevatron RunI data excludes $\mgl\leq 240$ GeV. Finally, we discuss application of the procedures developed for the heavy gluino-LSP to searches for other stable strongly interacting particles, such as a stable heavy quark.

Human review
References
How later papers used it

50 later papers cite it

Evidence: substantial. 50 of the citing papers share no author with it, and 6 of those carry a confident label from Pith's citation classifier.

Pith read 10 of the 69 citing sentences, choosing only those whose citation markers point at this paper alone, and wrote the paraphrases from them. The summary, the counts, the evidence level, the links and the quotes come from code; the summary counts the papers listed below. A later paper is listed under a label when Pith's citation classifier gives one of its sentences that label at probability 0.8 or more (0.95 for support), Pith's reading finds that the citing paper itself did it, and a second check confirms the paraphrase against the sentence. This section lists uses only. It does not list criticism or disagreement, so their absence here says nothing about how the paper has been received. Papers that share an author with this one are listed apart, under "By the same authors". A quote is the citing authors' own sentence, shown when their paper's licence is CC BY, CC BY-SA or CC0. JSON

Uses its data or values 1 of 5 papers with this label
  • Imposed experimental lower mass bounds on NLSPs in GMSB scenarios, including a gluino bound of 240.0 GeV from this paper.

    Parameter Space of General Gauge Mediation (2009) · 0.99 · paraphrased: the licence does not allow quoting

How the literature uses it

47 arXiv papers cite this in 65 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 · 41 sentences without a confident label

Uses its method or tool 1 paper
Uses its data or values 5 papers
  • We also impose the current experimental lower mass bounds on NLSPs in GMSB scenarios: neutralinos at 114.0 GeV, squarks at 250.0 GeV, sleptons at 87.4 GeV, charginos at 101.0 GeV, sneutrinos at 43.7 GeV [ref] , and gluinos 240.0 GeV [ref] .

    Parameter Space of General Gauge Mediation · The Minimal General Gauge Mediation Framework · 0.99

  • In this case, $k = 27/64$ [ref] , and $$, the hidden to visible temperature ratio at BBN, may be as large as 0.63.

    WIMPless Dark Matter from Non-Abelian Hidden Sectors with Anomaly-Mediated Supersymmetry Breaking · A Pure SU($N$) Hidden Sector without Connectors · 0.89

  • where $n_f$ is the number of quark flavors into which $Q$ can annihilate, and $(c_f,c_g)= (2/9,220/27)$ for triplets [ref] , $(3/2,27/4)$ for octets [ref] , etc.

    Window for preferred axion models · Abundance of strongly interacting relics · 0.92

Cites it as background 17 papers

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