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High Energy Physics - Phenomenology · arXiv:hep-ph/0504210 v3 · submitted 22 Apr 2005

Limits on Split Supersymmetry from Gluino Cosmology

A. Arvanitaki, C. Davis, P. W. Graham, A. Pierce, J. G. Wacker

PDF · arXiv · The abstract, sentence by sentence · Cite

The paper says

“An upper limit on the masses of scalar superpartners in split supersymmetry is found by considering cosmological constraints on long-lived gluinos.”

from the abstract · picked out as the main claim by a classifier

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The paper

Abstract

An upper limit on the masses of scalar superpartners in split supersymmetry is found by considering cosmological constraints on long-lived gluinos. Over most of parameter space, the most stringent constraint comes from big bang nucleosynthesis. A TeV mass gluino must have a lifetime of less than 100 seconds to avoid altering the abundances of D and Li-6. This sets an upper limit on the supersymmetry breaking scale of 10^9 GeV.

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. No sentence in this record was written by a model.

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

How the main claim is stated: asserted 1.00

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.26 · human participants 0.01 · controlled comparison 0.03 · 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

This table labels the abstract only (arXiv listing abstract v3). The number is the probability the classifier gave the label.

SentenceRoleThe authors' own workStates the main conclusionStrength
An upper limit on the masses of scalar superpartners in split supersymmetry is found by considering cosmological constraints on long-lived gluinos. result 0.65 0.87 0.78 asserted 1.00
Over most of parameter space, the most stringent constraint comes from big bang nucleosynthesis. result 0.87 0.64 0.08 asserted 0.98
A TeV mass gluino must have a lifetime of less than 100 seconds to avoid altering the abundances of D and Li-6. result 0.97 0.52 0.14 asserted 1.00
This sets an upper limit on the supersymmetry breaking scale of 10^9 GeV. result 0.95 0.82 0.64 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from argument 0.52

What was examined, and what was not

Sources read

  • arXiv listing abstract v3

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

How the labels were made

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,554 input tokens, $0.0001 reported.

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. This record as JSON

Cited by 19 Pith papers

Reviewed papers on Pith that cite this one. The full citation record

  1. Cosmological Abundance of Colored Relics hep-ph · Nov 2018
  2. Dark quarkonium formation in the early universe hep-ph · Feb 2018
  3. Colored Dark Matter hep-ph · Jan 2018
  4. Redefining the Axion Window hep-ph · Oct 2016
  5. Asymmetric Dark Matter from Leptogenesis hep-ph · Jan 2011
  6. Astrophysical Probes of Unification hep-ph · Dec 2008
  7. Minimal SO(10) splits supersymmetry hep-ph · Sep 2008
  8. The MSSM with heavy scalars hep-ph · May 2007
  9. The Relic Abundance of Long-lived Heavy Colored Particles hep-ph · Nov 2006
  10. Electric Dipole Moments in Split Supersymmetry hep-ph · Oct 2005
  11. Gluino Decays in Split Supersymmetry hep-ph · Jun 2005
  12. The number density of a charged relic hep-ph · Jul 2008
  13. Window for preferred axion models hep-ph · May 2017
  14. WIMPless Dark Matter from Non-Abelian Hidden Sectors with Anomaly-Mediated Supersymmetry Breaking hep-ph · Feb 2011
  15. Dark Matter Through the Neutrino Portal hep-ph · Aug 2009
  16. Probing seesaw at LHC hep-ph · Mar 2007
  17. Les Houches "Physics at TeV Colliders 2005'' Beyond the Standard Model working group: summary report hep-ph · Feb 2006
  18. Non-collider searches for stable massive particles hep-ph · Oct 2014
  19. Stable Massive Particles at Colliders hep-ph · Nov 2006
How the literature uses it

27 arXiv papers cite this in 40 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 · 33 sentences without a confident label

Builds on it 1 paper
  • We extend the discussions of Refs. [ref] , held in the context of universal gaugino masses, to the various scenarios with non-universal boundary conditions at $M_GUT$.

    The MSSM with heavy scalars · The gluino lifetime · 1.00

Uses its data or values 2 papers
  • The gluino mass range that gives the measured $$ abundance is $300-7000$ GeV [ref] .

    Astrophysical Probes of Unification · Split SUSY · 0.98

  • In this section we analyze the constraints on the MSSM with heavy scalars, first from collider searches and high-precision data [ref] and then from cosmological data, in particular the relic density measurement of DM by the WMAP satellite [ref] and the gluino lifetime [ref] .

    The MSSM with heavy scalars · Collider and Dark Matter constraints · 0.84

Cites it as background 4 papers
  • Stable “colored” particles, charged under QCD or a hidden confining gauge group, have been proposed as dark matter (DM) candidates [ref] , and are predicted in various extensions of the Standard Model [ref] .

    Dark quarkonium formation in the early universe · Introduction · 0.96

  • Constraints from cosmology on such kind of hadronic states have been mostly studied for the case of a stable exotic quark [ref] , a gluino LSP [ref] or for very long-lived gluino in the split SUSY scenarios [ref] .

    The number density of a charged relic · Unitarity bound · 0.90

  • Cosmologically long-lived gluinos were reconsidered in [ref] .

    Window for preferred axion models · Abundance of strongly interacting relics · 0.80

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