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Neutralino dark matter confronted by the LHC constraints on Electroweak SUSY signals

High Energy Physics - Phenomenology · Submitted 4 May 2013

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

The authors' main claim It is shown that even the preliminary data on the direct searches of these sparticles at the LHC, significantly constrain the parameter space of the MSSM compatible with the observed relic density and provide useful hints about the future search prospects.

how it is stated · asserted 1.00 read the record →

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arXiv ID1305.0928 (version 3)
Pith IDKSHXBW2L, Pith's permanent record of this paper and its review
CitationAmitava Datta, Arghya Choudhury. "Neutralino dark matter confronted by the LHC constraints on Electroweak SUSY signals." arXiv:1305.0928 (2013). https://pith.science/paper/KSHXBW2L
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, 6,457 input tokens, $0.0003 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.31 · human participants 0.01 · controlled comparison 0.15 · randomized assignment 0.01 · states quantitative result 0.96 · compares with prior results 0.87 · mentions code or data availability 0.03.

The abstract, sentence by sentence

arXiv listing abstract v3. Results and the main claim are underlined; .

The supersymmetric particles (sparticles) belonging exclusively to the electroweak sector of the minimal supersymmetric standard model (MSSM) may hold the key to the observed dark matter relic density in the universe even if all strongly interacting sparticles are very heavy. The importance of the light EW sparticles in DM physics and in producing spectacular collider signals is emphasized. It is shown that even the preliminary data on the direct searches of these sparticles at the LHC, significantly constrain the parameter space of the MSSM compatible with the observed relic density and provide useful hints about the future search prospects. If in addition to the electroweak sparticles the gluinos are also within the reach of the LHC experiments, then the gluino mass limits in the light slepton scenario obtained via the canonical jets + $\met$ channel may be relaxed by as much as 25 $%$ compared to the existing limits. But the corresponding same sign dilepton (SSD) + jets + $\met$ signal will yield enhanced limits competitive with the strongest limits currently available. This is illustrated with the help of benchmark scenarios at the generator level using PYTHIA. If the gluinos are just beyond the current reach of the LHC, then the generic n-lepton + m-jets + missing energy signal may discriminate between different DM producing mechanisms by comparing the signals corresponding to different values of n. This is illustrated by simulating the signals for n = 0 and n = 2 (the SSD signal).

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 The supersymmetric particles (sparticles) belonging exclusively to the electroweak sector of the minimal supersymmetric standard model (MSSM) may hold the key to the observed dark matter relic density in the universe even if all strongly interacting sparticles are very heavy. background 0.99 0.10 0.14 hedged possibility 1.00
s1 The importance of the light EW sparticles in DM physics and in producing spectacular collider signals is emphasized. background 0.67 0.18 0.08 asserted 0.96
s2 It is shown that even the preliminary data on the direct searches of these sparticles at the LHC, significantly constrain the parameter space of the MSSM compatible with the observed relic density and provide useful hints about the future search prospects. result 0.94 0.83 0.66 asserted 1.00
s3 If in addition to the electroweak sparticles the gluinos are also within the reach of the LHC experiments, then the gluino mass limits in the light slepton scenario obtained via the canonical jets + $\met$ channel may be relaxed by as much as 25 $%$ compared to the existing limits. result 0.98 0.68 0.12 hedged possibility 0.95
s4 But the corresponding same sign dilepton (SSD) + jets + $\met$ signal will yield enhanced limits competitive with the strongest limits currently available. result 0.96 0.61 0.12 asserted 0.87
s5 This is illustrated with the help of benchmark scenarios at the generator level using PYTHIA. method 1.00 0.85 0.03 asserted 0.96
s6 If the gluinos are just beyond the current reach of the LHC, then the generic n-lepton + m-jets + missing energy signal may discriminate between different DM producing mechanisms by comparing the signals corresponding to different values of n. result 0.51 0.42 0.10 hedged possibility 1.00
s7 This is illustrated by simulating the signals for n = 0 and n = 2 (the SSD signal). method 0.96 0.86 0.05 asserted 0.95

What kind of paper the classifier reports this is: simulation study 0.97 · evidence from simulation or computation 0.86.

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

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

The supersymmetric particles (sparticles) belonging exclusively to the electroweak sector of the minimal supersymmetric standard model (MSSM) may hold the key to the observed dark matter relic density in the universe even if all strongly interacting sparticles are very heavy. The importance of the light EW sparticles in DM physics and in producing spectacular collider signals is emphasized. It is shown that even the preliminary data on the direct searches of these sparticles at the LHC, significantly constrain the parameter space of the MSSM compatible with the observed relic density and provide useful hints about the future search prospects. If in addition to the electroweak sparticles the gluinos are also within the reach of the LHC experiments, then the gluino mass limits in the light slepton scenario obtained via the canonical jets + $\met$ channel may be relaxed by as much as 25 $%$ compared to the existing limits. But the corresponding same sign dilepton (SSD) + jets + $\met$ signal will yield enhanced limits competitive with the strongest limits currently available. This is illustrated with the help of benchmark scenarios at the generator level using PYTHIA. If the gluinos are just beyond the current reach of the LHC, then the generic n-lepton + m-jets + missing energy signal may discriminate between different DM producing mechanisms by comparing the signals corresponding to different values of n. This is illustrated by simulating the signals for n = 0 and n = 2 (the SSD signal).

Human review
References
How the literature uses it

24 arXiv papers cite this in 29 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 · 14 sentences without a confident label

Uses its method or tool 1 paper
Cites it as support 1 paper
Cites it as background 13 papers

What it cites · 56 sentences without a confident label

Builds on 2 papers
Uses the method or tool of 6 papers
Uses data or values from 8 papers
Compares with 1 paper
  • Recently this model has been constrained by simultaneously using the ATLAS data on chargino - neutralino search and the $(g-2)_μ$ data (see Figs. 1(a) - 1(c) of [ref] ) These constraints can not be directly compared with the similar ones obtained by ATLAS [ref] , as they were obtained with different MSSM inputs.

    Muon g-2 vs LHC in Supersymmetric Models · Collider Signals and Other Observables · 0.83

Cites as background 17 papers

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