{"arxiv_id":"1202.1503","incoming":{"papers":29,"sentences":49,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":7,"sentences":9,"quotes":[{"arxiv_id":"1302.5956","title":"Two ultimate tests of constrained supersymmetry","url":"/paper/1302.5956","section":"Scanning Methodology and Constraints","sentence":"We follow the procedure outlined in detail in Refs. [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"1207.4930","title":"Global Study of the Simplest Scalar Phantom Dark Matter Model","url":"/paper/1207.4930","section":"Indirect Detection","sentence":"Since each limit was obtained by assuming the dominance by one single channel, we can approximately reconstruct the upper limit suitable to our case by applying the same method as in Sec. 4.1 of [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"1211.1693","title":"The Constrained NMSSM with a 126 GeV Higgs boson: A global analysis","url":"/paper/1211.1693","section":"Statistical treatment of experimental data","sentence":"We follow the procedure outlined in detail in our previous papers [ref] , of which we give a short summary here.","intent_p":1.0,"contests_p":null},{"arxiv_id":"2403.02721","title":"Light Thermal Dark Matter Beyond $p$-Wave Annihilation in Minimal Higgs Portal Model","url":"/paper/2403.02721","section":"result","sentence":"To reconstruct the future sensitivity of the e-ASTROGAM for any given annihilation final state, we adopt the approach developed in Ref. [ref] to compute the $95%$ upper limit on the photon flux induced by DM annihilation.","intent_p":1.0,"contests_p":null},{"arxiv_id":"1405.4289","title":"What next for the CMSSM and the NUHM: Improved prospects for superpartner and dark matter detection","url":"/paper/1405.4289","section":"Scanning methodology and experimental constraints","sentence":"We follow a Bayesian approach outlined in [ref] and map out the $68%$ and $95%$ credible regions in two-dimensional (2D) projections of the marginalized posterior probability density function (pdf) and/or the one-dimensional (1D) marginalized pdf of some interesting parameters.","intent_p":1.0,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1406.1181","title":"Light Neutralino Dark Matter: Direct/Indirect Detection and Collider Searches","url":"/paper/1406.1181","section":"Relic Abundance Considerations","sentence":"As for a rather tight requirement, we demand the calculated relic density corresponding to the 2$σ$ window of the observed relic density [ref] plus $10%$ theoretical uncertainty [ref] .","intent_p":0.91,"contests_p":null},{"arxiv_id":"1303.3040","title":"Dark matter and Higgs bosons in the MSSM","url":"/paper/1303.3040","section":"Introduction","sentence":"The non-observation of gamma rays from DM annihilation in the nearby dwarf galaxies [ref] has been used to place constraints on the DM particle mass $m_χ≳40$ GeV, for neutralino annihilation to the $b b̅$ channel with a velocity-independent cross section $=$ 1 pb$×$c, although these bounds would be relaxed with a more general analysis including the velocity-dependent contributions [ref] .","intent_p":0.82,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":2,"sentences":6,"quotes":[{"arxiv_id":"1206.0264","title":"Constrained MSSM favoring new territories: The impact of new LHC limits and a 125 GeV Higgs boson","url":"/paper/1206.0264","section":"The CMSSM with","sentence":"Most notably, the high probability mode which, in that paper and in Ref. [ref] , was spread over the focus point (FP)/hyperbolic branch (HB) region at large and $≪$, has now moved up to the $A$-funnel region.","intent_p":1.0,"contests_p":null},{"arxiv_id":"1204.4199","title":"Constrained Supersymmetry after two years of LHC data: a global view with Fittino","url":"/paper/1204.4199","section":"Introduction","sentence":"Technically, the methods employed to obtain the results presented in this paper differ in various aspects from our previous studies [ref] and from those used in other global fits with LHC exclusions [ref] .","intent_p":0.83,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1302.5956","title":"Two ultimate tests of constrained supersymmetry","url":"/paper/1302.5956","section":"The CMSSM","sentence":"However, as demonstrated in [ref] and mentioned above, this region is probably not yet firmly excluded due to large theoretical and astrophysical uncertainties.","intent_p":0.97,"contests_p":null},{"arxiv_id":"1211.1693","title":"The Constrained NMSSM with a 126 GeV Higgs boson: A global analysis","url":"/paper/1211.1693","section":"Prospects for DM direct detection and","sentence":"We want to point out that the theory uncertainties are very large (up to a factor of 10) and strongly affect the impact of the experimental limit on the parameter space [ref] .","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":8,"sentences":9,"quotes":[{"arxiv_id":"1712.04793","title":"Identifying WIMP dark matter from particle and astroparticle data","url":"/paper/1712.04793","section":"Introduction","sentence":"[ref] ), typically within the context of a global fitting analysis [ref] .","intent_p":0.93,"contests_p":null},{"arxiv_id":"1205.1568","title":"Should we still believe in constrained supersymmetry?","url":"/paper/1205.1568","section":"Introduction","sentence":"In the Bayesian approach model selection is based on the Bayes factor, and requires comparison to alternative hypotheses [ref] .","intent_p":0.86,"contests_p":null},{"arxiv_id":"1203.5048","title":"Higgs bosons near 125 GeV in the NMSSM with constraints at the GUT scale","url":"/paper/1203.5048","section":"Introduction","sentence":"Since then, several publications have studied the impact of a Higgs boson in the 125 GeV range on the parameter space of supersymmetric (Susy) extensions of the SM [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"1912.04079","title":"GAMBIT and its Application in the Search for Physics Beyond the Standard Model","url":"/paper/1912.04079","section":"Supersymmetry","sentence":"The has been studied in global fits for over a decade [ref] , most recently in the analysis in [ref] .","intent_p":0.9,"contests_p":null},{"arxiv_id":"1705.07908","title":"GAMBIT: The Global and Modular Beyond-the-Standard-Model Inference Tool","url":"/paper/1705.07908","section":"Introduction","sentence":"Several attempts to address this problem have been made in particle physics, from the characterisation of electroweak physics with [ref] and later [ref] to CKM fits [ref] , neutrino global fits [ref] and global analyses of supersymmetry (SUSY) [ref] , in particular with packages like [ref] , [ref] , [ref] and others [ref] .","intent_p":0.91,"contests_p":null}]}],"unlabelled_sentences":21},"outgoing":{"papers":39,"sentences":113,"groups":[{"kind":"extends","label":"Builds on","papers":1,"sentences":3,"quotes":[{"arxiv_id":"1111.6098","title":"Bayesian Implications of Current LHC and XENON100 Search Limits for the Constrained MSSM","url":"/paper/1111.6098","section":"Introduction","sentence":"In this paper we look deeper into the FP/HB region and perform a Bayesian analysis of the CMSSM with its soft mass parameters extended to $m_0≤4$ TeV and $m_1/2≤2$ TeV, which is for each parameter twice as large as in [ref] .","intent_p":1.0,"contests_p":null}]},{"kind":"method_or_tool","label":"Uses the method or tool of","papers":5,"sentences":9,"quotes":[{"arxiv_id":"1111.6098","title":"Bayesian Implications of Current LHC and XENON100 Search Limits for the Constrained MSSM","url":"/paper/1111.6098","section":"The $α_T$ SUSY search","sentence":"In order to calculate the likelihood for the LHC signal, we generally follow the procedure detailed in Ref. [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"hep-ph/0602028","title":"A Markov Chain Monte Carlo Analysis of the CMSSM","url":"/paper/hep-ph/0602028","section":"XENON100 bound","sentence":"We include $τ$ in the likelihood, following the procedure described in [ref] for the treatment of upper bounds.","intent_p":1.0,"contests_p":null},{"arxiv_id":"astro-ph/0406204","title":"DarkSUSY: Computing Supersymmetric Dark Matter Properties Numerically","url":"/paper/astro-ph/0406204","section":"Neutrino telescopes","sentence":"Notice that SuperBayeS (following DarkSusy [ref] ) uses tables from WimpSim [ref] for the propagation of the neutrino flux through the Sun and to Earth, so that matter effects and neutrino oscillations are properly accounted for.","intent_p":0.99,"contests_p":null},{"arxiv_id":"0709.3898","title":"Neutrinos from WIMP Annihilations Obtained Using a Full Three-Flavor Monte Carlo Approach","url":"/paper/0709.3898","section":"Neutrino telescopes","sentence":"Notice that SuperBayeS (following DarkSusy [ref] ) uses tables from WimpSim [ref] for the propagation of the neutrino flux through the Sun and to Earth, so that matter effects and neutrino oscillations are properly accounted for.","intent_p":0.99,"contests_p":null},{"arxiv_id":"1004.4573","title":"Fermion WIMPless Dark Matter at DeepCore and IceCube","url":"/paper/1004.4573","section":"Neutrino telescopes","sentence":"In order to realistically approximate the detector response, we follow the procedure given in Appendix B of Ref. 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[ref] .","intent_p":0.9,"contests_p":null},{"arxiv_id":"1103.0303","title":"Likelihood Approach to the First Dark Matter Results from XENON100","url":"/paper/1103.0303","section":"XENON100 bound","sentence":"We incorporate in our scan the constraints induced on the SI neutralino-proton cross section $σ_p^SI$ by the 90% C.L. upper bound $σ_p,90^SI$, which was recently published by the XENON100 Collaboration [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1104.2549","title":"Dark Matter Results from 100 Live Days of XENON100 Data","url":"/paper/1104.2549","section":"XENON100 bound","sentence":"We incorporate in our scan the constraints induced on the SI neutralino-proton cross section $σ_p^SI$ by the 90% C.L. upper bound $σ_p,90^SI$, which was recently published by the XENON100 Collaboration [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1107.2155","title":"The XENON100 Dark Matter Experiment","url":"/paper/1107.2155","section":"XENON100 bound","sentence":"We incorporate in our scan the constraints induced on the SI neutralino-proton cross section $σ_p^SI$ by the 90% C.L. upper bound $σ_p,90^SI$, which was recently published by the XENON100 Collaboration [ref] .","intent_p":1.0,"contests_p":null}]},{"kind":"comparison","label":"Compares with","papers":5,"sentences":9,"quotes":[{"arxiv_id":"1111.6098","title":"Bayesian Implications of Current LHC and XENON100 Search Limits for the Constrained MSSM","url":"/paper/1111.6098","section":"Impact on the CMSSM parameter space","sentence":"First, we have checked that, without including the dSphs $γ$-ray constraint, our results agreed well with those of Ref. [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1110.3568","title":"Supersymmetry in Light of 1/fb of LHC Data","url":"/paper/1110.3568","section":"Introduction","sentence":"Reference [ref] adopted frequentist","intent_p":0.84,"contests_p":null},{"arxiv_id":"1107.1715","title":"Global fits of the cMSSM including the first LHC and XENON100 data","url":"/paper/1107.1715","section":"XENON100 bound","sentence":"Two recent papers [ref] also considered the impact of the XENON100 bound on CMSSM PS in the Bayesian framework but their treatment of the theoretical uncertainties differs from ours.","intent_p":0.83,"contests_p":null},{"arxiv_id":"1004.4573","title":"Fermion WIMPless Dark Matter at DeepCore and IceCube","url":"/paper/1004.4573","section":"Neutrino telescopes","sentence":"We compared our spectra and rates with the code used for the calculations performed in [ref] and found very good agreement.","intent_p":1.0,"contests_p":null},{"arxiv_id":"1103.5061","title":"New Constraints on Dark Matter from CMS and ATLAS Data","url":"/paper/1103.5061","section":"Introduction","sentence":"statistics and [ref] performed a fixed-grid scan in contrast to our Bayesian one, while Refs. 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[ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"0907.1486","title":"Prospects for Indirect Detection of Sneutrino Dark Matter with IceCube","url":"/paper/0907.1486","section":"Neutrino telescopes","sentence":"While presently available data do not allow us to draw any definite conclusions, the results for the full configuration (which should be published soon) will have significant constraining power, as noted already in Refs. [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"1105.5162","title":"The Quest for Supersymmetry: Early LHC Results versus Direct and Indirect Neutralino Dark Matter Searches","url":"/paper/1105.5162","section":"Neutrino telescopes","sentence":"While presently available data do not allow us to draw any definite conclusions, the results for the full configuration (which should be published soon) will have significant constraining power, as noted already in Refs. [ref] .","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":10,"sentences":10,"quotes":[{"arxiv_id":"1109.2352","title":"Search for Supersymmetry at the LHC in Events with Jets and Missing Transverse Energy","url":"/paper/1109.2352","section":"Introduction","sentence":"The Large Hadron Collider (LHC) at CERN started its run at center of mass energy $√(s)=7$ TeV more than a year ago, and in 2011 published several results based on an integrated luminosity of 1.1 fb$^-1$ [ref] .","intent_p":0.91,"contests_p":null},{"arxiv_id":"1109.6572","title":"Search for squarks and gluinos using final states with jets and missing transverse momentum with the ATLAS detector in sqrt(s) = 7 TeV proton-proton collisions","url":"/paper/1109.6572","section":"Introduction","sentence":"The Large Hadron Collider (LHC) at CERN started its run at center of mass energy $√(s)=7$ TeV more than a year ago, and in 2011 published several results based on an integrated luminosity of 1.1 fb$^-1$ [ref] .","intent_p":0.91,"contests_p":null},{"arxiv_id":"1110.3568","title":"Supersymmetry in Light of 1/fb of LHC Data","url":"/paper/1110.3568","section":"Introduction","sentence":"Recently, there have been many studies, both experimental and phenomenological, of the impact of bounds from new physics searches at the LHC on the parameter space (PS) of the CMSSM [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"1103.5061","title":"New Constraints on Dark Matter from CMS and ATLAS Data","url":"/paper/1103.5061","section":"Introduction","sentence":"Recently, there have been many studies, both experimental and phenomenological, of the impact of bounds from new physics searches at the LHC on the parameter space (PS) of the CMSSM [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"1107.1715","title":"Global fits of the cMSSM including the first LHC and XENON100 data","url":"/paper/1107.1715","section":"Introduction","sentence":"Recently, there have been many studies, both experimental and phenomenological, of the impact of bounds from new physics searches at the LHC on the parameter space (PS) of the CMSSM [ref] .","intent_p":0.96,"contests_p":null}]}],"unlabelled_sentences":63},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":null,"_links":{"html":"https://pith.science/paper/1202.1503"}}