{"arxiv_id":"1007.1151","incoming":{"papers":28,"sentences":38,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1309.6359","title":"A Singlet Extension of the MSSM with a Dark Matter Portal","url":"/paper/1309.6359","section":"$Γ^inv_Z$ and Neutralino sector","sentence":"To calculate the cross section we follow the analysis in [ref] where [equation] $s=209.^2$ GeV$^2$ is the center of mass energy at LEP 2 and $N_ij$ is the matrix that diagonalizes the neutralino weak eigenstates introduced in Equation ([ref]).","intent_p":0.99,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1703.00343","title":"Light Neutralino Dark Matter in the NMSSM","url":"/paper/1703.00343","section":"Collider Constraints","sentence":"The invisible decay width $Γ^inv_Z$ is determined by [ref] , [equation] The reported experimental bound $Γ^inv_Z≤2$ MeV [ref] implies that the magnitude of $(N^2_13-N^2_14)^2$ in Eq.([ref]) is upper bounded by $∼0.01$ roughly.","intent_p":0.81,"contests_p":null},{"arxiv_id":"1009.2555","title":"CoGeNT, DAMA, and Neutralino Dark Matter in the Next-To-Minimal Supersymmetric Standard Model","url":"/paper/1009.2555","section":"Constraints and Scanning in the NMSSM","sentence":"However, we have updated the limit on $Γ_Z→$ to $1.9$ as in [ref] .] We have augmented to include the recent ALEPH constraints [ref] on $→Z +Higgs$ with $Higgs→aa$ (in our case $a=$, the lightest CP-odd Higgs boson of the NMSSM) with $a→$.","intent_p":0.85,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":4,"sentences":6,"quotes":[{"arxiv_id":"1009.0549","title":"CoGeNT, DAMA, and Light Neutralino Dark Matter","url":"/paper/1009.0549","section":"Introduction","sentence":"Nonetheless they are “only” a factor of 10 too small (whereas in Ref. [ref] the largest cross section found was a factor of 100 too small).","intent_p":0.86,"contests_p":null},{"arxiv_id":"1107.1604","title":"Is light neutralino as dark matter still viable?","url":"/paper/1107.1604","section":"Summary","sentence":"However, we found that many of these points possessed too large a bino fraction to survive the flavour physics constraints, particularly that coming from $$, that we later re-invoked as $2σ$ hard cuts, finding results very similar to those obtained in [ref] where $10^-6$.","intent_p":0.97,"contests_p":null},{"arxiv_id":"1009.2555","title":"CoGeNT, DAMA, and Neutralino Dark Matter in the Next-To-Minimal Supersymmetric Standard Model","url":"/paper/1009.2555","section":"Benchmark Models In The NMSSM","sentence":"The larger $m_H_d-like$ in the scans of [ref] imply a larger $$ with the consequence that their largest $$ points are within the nominal $±2σ$ constraints from $b→s$ whereas our high-$$, $>0$ points are about $0.5σ$ outside the $±2σ$ region.","intent_p":1.0,"contests_p":null},{"arxiv_id":"1010.1789","title":"The Higgs Sector and CoGeNT/DAMA-Like Dark Matter in Supersymmetric Models","url":"/paper/1010.1789","section":"The Inverted Higgs Scenarios","sentence":"Finally, let me note that in the NMSSM study of [ref] cross sections as large as those found here are not achieved; rather, they find $^Max_SI∼(1-1.5)×10^-6$ (without enhancing the $s$-quark content of the nucleon).","intent_p":1.0,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":13,"sentences":13,"quotes":[{"arxiv_id":"2012.04026","title":"A relatively light, highly bino-like dark matter in the $Z_3$-symmetric NMSSM and recent LHC searches","url":"/paper/2012.04026","section":"Introduction","sentence":"Some later studies [ref] concentrated on a light bino-like DM ($≲40$ GeV, down to a few hundreds of MeV) that funnels through such light scalar(s) and were mostly motivated by the then recent reported excesses at experiments like DAMA, CoGeNT and CDMS-II and the exclusion limits from XENON and CDMS-Si experiments which all seemed to be compatible with such excesses.","intent_p":0.84,"contests_p":null},{"arxiv_id":"2010.11674","title":"Status of low mass LSP in SUSY","url":"/paper/2010.11674","section":"The neutralino $$ DM","sentence":"The case of a light $$ has been discussed in the literature extensively [ref] [In addition to these we already discussed the extensions of the NMSSM where a $ν_R$ can be a thermal DM candidate and leads to characteristic LHC signals.].","intent_p":0.83,"contests_p":null},{"arxiv_id":"1612.00460","title":"Low-mass neutralino dark matter in supergravity scenarios: phenomenology and naturalness","url":"/paper/1612.00460","section":"Introduction","sentence":"Light neutralino DM has been studied in the most appealing realisations of Supersymmetry (SUSY) at the Electroweak (EW) scale such as the Minimal Supersymmetric Standard Model (MSSM) [ref] , the Next-to-MSSM (NMSSM) [ref] , and some minimal extensions of the NMSSM [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"1307.7601","title":"Collider signatures of a light NMSSM pseudoscalar in neutralino decays in the light of LHC results","url":"/paper/1307.7601","section":"Light Higgs scenarios in the NMSSM and choice of benchmark points","sentence":"In terms of the field content, the singlet mixes with the doublet Higgs states, giving rise to three CP-even $(1, 2, 3)$ and two CP-odd $(1, 1)$ states, whereas the singlino mixes with the neutralinos, inducing a fifth eigenstate $(_1, …, _5)$, with interesting implications for dark matter searches (see, e.g., Refs. [ref] ).","intent_p":0.98,"contests_p":null},{"arxiv_id":"1703.01255","title":"Perspectives of direct Detection of supersymmetric Dark Matter in the NMSSM","url":"/paper/1703.01255","section":"Introduction","sentence":"The larger diversity of the LSP properties has led to many studies of direct DM detection in the NMSSM, see e.g. [ref] .","intent_p":0.95,"contests_p":null}]}],"unlabelled_sentences":16},"outgoing":{"papers":56,"sentences":88,"groups":[{"kind":"contests","label":"Contests","papers":1,"sentences":1,"quotes":[{"arxiv_id":"hep-ph/0509024","title":"Light Neutralino Dark Matter in the NMSSM","url":"/paper/hep-ph/0509024","section":"Introduction","sentence":"However, the corresponding points in the parameter space given as examples in [ref] suffer from a negative effective $μ$-parameter (which is in conflict with the measured anomalous magnetic moment of the muon), and not all experimental constraints considered below are taken into 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