{"arxiv_id":"1011.6108","incoming":{"papers":8,"sentences":12,"groups":[{"kind":"background","label":"Cites it as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1803.10977","title":"Effects of Threshold Energy on Reconstructions of Properties of Low-Mass WIMPs in Direct Dark Matter Detection Experiments","url":"/paper/1803.10977","section":"Introduction","sentence":"Different methods have been purposed for reconstructing the WIMP mass $$ [ref] and spin–independent (SI)/spin–dependent (SD) WIMP–nucleon cross sections $σ_χ(p, n)^SI, SD$ [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"1304.1758","title":"Complementarity of dark matter direct detection: the role of bolometric targets","url":"/paper/1304.1758","section":"Introduction","sentence":"The idea of target complementarity has later been applied to the determination of the WIMP mass and cross section from different DM experiments [ref] and the relevance of targets sensitive to the SD cross section has been analytically studied in Ref. [ref] .","intent_p":0.88,"contests_p":null}]}],"unlabelled_sentences":10},"outgoing":{"papers":37,"sentences":60,"groups":[{"kind":"method_or_tool","label":"Uses the method or tool of","papers":4,"sentences":4,"quotes":[{"arxiv_id":"hep-ph/0005041","title":"A New Model-Independent Method for Extracting Spin-Dependent Cross Section Limits from Dark Matter Searches","url":"/paper/hep-ph/0005041","section":"Discussion","sentence":"As a matter of fact, has become a standard procedure to use the method of Ref. [ref] to set limits on the cross sections in a WIMP-independent way.","intent_p":0.84,"contests_p":null},{"arxiv_id":"1003.5164","title":"Impact of internal bremsstrahlung on the detection of gamma-rays from neutralinos","url":"/paper/1003.5164","section":"Comparison with the CMSSM","sentence":"We further impose [ref] the LEP bound on the light Higgs mass $m_h >114$ GeV, and other phenomenological constraints using the code [ref] .","intent_p":0.81,"contests_p":null},{"arxiv_id":"hep-ph/0012020","title":"Cold Dark Matter detection in SUSY models at large tan(beta)","url":"/paper/hep-ph/0012020","section":"Comparison with the CMSSM","sentence":"We further impose [ref] the LEP bound on the light Higgs mass $m_h >114$ GeV, and other phenomenological constraints using the code [ref] .","intent_p":0.81,"contests_p":null},{"arxiv_id":"astro-ph/0406204","title":"DarkSUSY: Computing Supersymmetric Dark Matter Properties Numerically","url":"/paper/astro-ph/0406204","section":"Comparison with the CMSSM","sentence":"We further impose [ref] the LEP bound on the light Higgs mass $m_h >114$ GeV, and other phenomenological constraints using the code [ref] .","intent_p":0.81,"contests_p":null}]},{"kind":"data_used","label":"Uses data or values from","papers":5,"sentences":8,"quotes":[{"arxiv_id":"hep-ph/9702290","title":"Spin-Dependent Neutralino-Nucleus Scattering for $A \\sim 127$ Nuclei","url":"/paper/hep-ph/9702290","section":"An analytical scheme for extracting the elementary cross sections","sentence":"For $^19$F we use the spin matrix elements of Ref. [ref] that give $Ω^19_p =1.646$ and $Ω^19_n = -0.030$; for $^73$Ge the results of Ref. [ref] , $Ω^73_p =0.066$ and $Ω^73_n = 0.836$; finally for $^127$I the set obtained with the potential Bonn-A from Ref. [ref] that furnishes $Ω^127_p =0.731$ and $Ω^127_n =0.177$.","intent_p":1.0,"contests_p":null},{"arxiv_id":"hep-ph/9408246","title":"Scatttering of Weakly Interacting Massive Particles from Ge73","url":"/paper/hep-ph/9408246","section":"An analytical scheme for extracting the elementary cross sections","sentence":"For $^19$F we use the spin matrix elements of Ref. [ref] that give $Ω^19_p =1.646$ and $Ω^19_n = -0.030$; for $^73$Ge the results of Ref. [ref] , $Ω^73_p =0.066$ and $Ω^73_n = 0.836$; finally for $^127$I the set obtained with the potential Bonn-A from Ref. [ref] that furnishes $Ω^127_p =0.731$ and $Ω^127_n =0.177$.","intent_p":1.0,"contests_p":null},{"arxiv_id":"0907.3587","title":"Searching for Dark Matter- Theoretical Rates and Exclusion Plots due to the Spin","url":"/paper/0907.3587","section":"An analytical scheme for extracting the elementary cross sections","sentence":"In the specific case of $^127$I, $^73$Ge, $^19$F, the factors $t^SI,SD$ were calculated for $E_min=0$ and neutralino masses up to 200 GeV in Ref. [ref] .","intent_p":0.91,"contests_p":null},{"arxiv_id":"hep-ex/0609039","title":"Precise determination of the spin structure function $\\mathbf{g_1}$ of the proton, deuteron and neutron","url":"/paper/hep-ex/0609039","section":"Comparison with the CMSSM","sentence":"We adopted for the latter quantities the central values obtained by the HERMES collaboration for the proton [ref] , $u^(p) = 0.842$, $d^(p) = -0.427$, $s^(p) = -0.085$ and $u^(n) = d^(p)$, $d^(n) = u^(p)$, $s^(n) = s^(p)$ from isospin symmetry for the neutron.","intent_p":1.0,"contests_p":null},{"arxiv_id":"1001.4635","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters","url":"/paper/1001.4635","section":"Comparison with the CMSSM","sentence":"Assuming that the neutralino constitutes all the DM relic density as deduced from WMAP [ref] measurements, $0.094 < Ωh^2 < 0.128$ at 3$σ$, the CMSSM parameter space is heavily restricted.","intent_p":0.95,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":14,"sentences":14,"quotes":[{"arxiv_id":"hep-ph/9307208","title":"Neutralino-Nucleon Scattering Revisited","url":"/paper/hep-ph/9307208","section":"Introduction","sentence":"Neutralino scattering with nucleons [ref] arises at the elementary level from its interactions with quarks.","intent_p":0.94,"contests_p":null},{"arxiv_id":"hep-ph/9504320","title":"SEARCHING FOR COLD DARK MATTER","url":"/paper/hep-ph/9504320","section":"Introduction","sentence":"Neutralino scattering with nucleons [ref] arises at the elementary level from its interactions with quarks.","intent_p":0.94,"contests_p":null},{"arxiv_id":"0806.3917","title":"Direct Search for Dark Matter - Striking the Balance - and the Future","url":"/paper/0806.3917","section":"Introduction","sentence":"Other multi-couplings/multi-targets approaches and analysis are found in literature [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"astro-ph/0408346","title":"Can WIMP Spin Dependent Couplings explain DAMA data, in light of Null Results from Other Experiments?","url":"/paper/astro-ph/0408346","section":"Introduction","sentence":"An analysis of the experiments with SD sensitivity, in terms of both the SD proton and neutron cross section, was performed for example in Refs. [ref] .","intent_p":0.85,"contests_p":null},{"arxiv_id":"hep-ph/0404010","title":"Model-independent assessment of current direct searches for spin-dependent dark matter","url":"/paper/hep-ph/0404010","section":"Introduction","sentence":"An analysis of the experiments with SD sensitivity, in terms of both the SD proton and neutron cross section, was performed for example in Refs. [ref] .","intent_p":0.85,"contests_p":null}]}],"unlabelled_sentences":34},"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/1011.6108"}}