High Energy Physics - Phenomenology · arXiv:1007.4812 v2 · submitted 27 Jul 2010
Exploring SUSY light Higgs boson scenarios via dark matter experiments
The paper says
“Our analysis shows that most part of the A pole region can produce detectable gamma-rays and antiproton signals, and still be compatible with with recent direct detection data from XENON100 and CDMS-II.”
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The paper
Abstract
We examine the dark matter phenomenology in supersymmetric light higgs boson scenarios, adapting nonuniversal Higgs masses at the gauge coupling unification scale. The correct relic density is obtained mostly through the annihilation into a pseudoscalar A, which gives high values for the self-annihilation cross-section at present times. Our analysis shows that most part of the A pole region can produce detectable gamma-rays and antiproton signals, and still be compatible with with recent direct detection data from XENON100 and CDMS-II.
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abstract compiled · 2026-09-23 · no language-model review
How the main claim is stated: asserted 0.84
What the abstract itself states, as probabilities: claims first 0.02 · states limitation 0.19 · human participants 0.01 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.12 · compares with prior results 0.21 · mentions code or data availability 0.02
The abstract, sentence by sentence
This table labels the abstract only (arXiv listing abstract v2). The number is the probability the classifier gave the label.
| Sentence | Role | The authors' own work | States the main conclusion | Strength |
|---|---|---|---|---|
| We examine the dark matter phenomenology in supersymmetric light higgs boson scenarios, adapting nonuniversal Higgs masses at the gauge coupling unification scale. | contribution 0.97 | 0.82 | 0.05 | asserted 0.82 |
| The correct relic density is obtained mostly through the annihilation into a pseudoscalar $A$, which gives high values for the self-annihilation cross-section at present times. | result 0.93 | 0.70 | 0.17 | asserted 0.97 |
| Our analysis shows that most part of the $A$ pole region can produce detectable gamma-rays and antiproton signals, and still be compatible with with recent direct detection data from XENON100 and CDMS-II. | result 0.99 | 0.92 | 0.71 | asserted 0.84 |
What kind of paper the classifier reports this is: theoretical result 0.56 · evidence from simulation or computation 0.88
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- references and citing sentences
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- P abstract
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- S sections
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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,033 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 3 Pith papers
Reviewed papers on Pith that cite this one. The full citation record
How the literature uses it
9 arXiv papers cite this in 11 sentences
Papers citing it · 10 sentences without a confident label
Cites it as background 1 paper
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The dark matter phenomenology of NUHM models has been studied by several authors [ref] .
Flavored Co-annihilations · Flavored Co-annihilation in $δ$-NUHM · 0.99
What it cites · 56 sentences without a confident label
Uses the method or tool of 5 papers
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The parameters $μ$ and the sparticle spectrum have been computed with SuSpect [ref] .
SuSpect: a Fortran Code for the Supersymmetric and Higgs Particle Spectrum in the MSSM · The NUHM and low energy constraints · 1.00
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In this work, we shall use the two-zone diffusion model and its semi-analytical solution as described, for example, in references [ref] .
Full calculation of clumpiness boost factors for antimatter cosmic rays in the light of Lambda-CDM N-body simulation results · Antiproton Detection · 1.00
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In this work, we shall use the two-zone diffusion model and its semi-analytical solution as described, for example, in references [ref] .
Transport of exotic anti-nuclei: I- Fast formulae for antiproton fluxes · Antiproton Detection · 1.00
Uses data or values from 6 papers
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An important virtue is that with this new window, a light Higgs mass with $m_h ∼(95-100)$ GeV could explain the slight excess of events of $2.3σ$ statistical significance [ref] as reported by the LEP2 experiments [ref] .
A Supersymmetric Explanation of the Excess of Higgs-Like Events at LEP · Introduction · 0.80
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An important virtue is that with this new window, a light Higgs mass with $m_h ∼(95-100)$ GeV could explain the slight excess of events of $2.3σ$ statistical significance [ref] as reported by the LEP2 experiments [ref] .
Search for the Standard Model Higgs Boson at LEP · Introduction · 0.80
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* WMAP constraint : In computing the relic density constraint, we consider the following 3$σ$ limit of the WMAP data [ref] , [equation] Here $Ω_CDMh^2$ is the dark matter relic density in units of the critical density and $h=0.71±0.026$ is the Hubble constant in units of $100 Km s^-1 Mpc^-1$.
Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation · The NUHM and low energy constraints · 1.00
Compares with 1 paper
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In Fig.[ref] we depict the WMAP-compliant parameter points on the $(m_χ^0_1, σ_χ^0_1-N^SI)$ (neutralino mass - neutralino-nucleon spin-independent scattering cross-section) plane and compare them against the three strongest bounds available in the literature: The combined 2008 and 2009 CDMS-II [ref] results, the constraints from the XENON10 experiment as well as the latest bounds from XENON100.
Results from the Final Exposure of the CDMS II Experiment · Discussion on the constraints from Direct Detection experiments · 0.94
Cites as background 16 papers
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[ref] , a systematic study of the hadronic uncertainties entering the neutralino-nucleon scattering cross-section is performed.
Hadronic Uncertainties in the Elastic Scattering of Supersymmetric Dark Matter · Discussion on the constraints from Direct Detection experiments · 0.82
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Now, in the MSSM, the coupling $g_ZZh$ is not identical with the respective coupling in the SM, it can rather be written as $sin(β-α)g^SM_ZZh$(For reviews see [ref] ).
The Anatomy of Electro-Weak Symmetry Breaking. II: The Higgs bosons in the Minimal Supersymmetric Model · Introduction · 0.95
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Such treatments have of course been applied in the case of the MSSM neutralino dark matter detection [ref] .
The cosmic ray positron excess and neutralino dark matter · Antiproton Detection · 0.83
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