{"arxiv_id":"hep-ph/0406218","incoming":{"papers":32,"sentences":55,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2608.24791","title":"Probing Dirac Dark Matter in Composite Higgs Models with Xenon and Argon targets","url":"/paper/2608.24791","section":"Differential cross section","sentence":"For the subsequent analysis of the LDCP scattering on Xe isotopes with non-zero spin, we use the Odd Group Model (OGM) [ref] (for a review, see [ref] ), which implies that only one unpaired nucleon contribute to the nucleus spin $J$.","intent_p":0.83,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":12,"sentences":15,"quotes":[{"arxiv_id":"1812.09325","title":"Foraging for dark matter in large volume liquid scintillator neutrino detectors with multiscatter events","url":"/paper/1812.09325","section":"Cross section reach with existing triggers","sentence":"We have taken the values ${J_A, ⟨S_p ⟩, ⟨S_n ⟩} = {1/2, -0.026, -0.155}$ for $^13$C [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1803.08044","title":"Saturated Overburden Scattering and the Multiscatter Frontier: Discovering Dark Matter at the Planck Mass and Beyond","url":"/paper/1803.08044","section":"Prospects for Multiscatter Detection","sentence":"Following [ref] we take $(J_A, ⟨S_p ⟩, ⟨S_n ⟩)=(1/2, 0.01, 0.3)$ for $^129$Xe, $(3/2, -0.04, -0.24)$ for $^131$Xe, and $(1/2, 0.48, -0.01)$ for $^19$F.","intent_p":1.0,"contests_p":null},{"arxiv_id":"1805.06113","title":"Present and projected sensitivities of Dark Matter direct detection experiments to effective WIMP-nucleus couplings","url":"/paper/1805.06113","section":"Nuclear response functions for Caesium and Tungsten","sentence":"For $^183$W and $^333$Cs we take $<S_p>$=0, $<S_n>$=-0.17, and $<S_p>$=-0.37, $<S_n>$=0.003, respectively, both from Appendix C of Ref. [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1804.01231","title":"Dark Matter implications of DAMA/LIBRA-phase2 results","url":"/paper/1804.01231","section":"Results","sentence":"This is again due to the spin carried by the neutrons and protons, respectively, and the required balance between scattering off sodium and iodine in order to yield an energy dependence of the signal matching the DAMA/LIBRA data: The ratio of the spin carried by the neutrons at zero momentum for sodium and iodine is $⟨S_n^Na⟩/⟨S_n^I⟩∼0.3$, while the ratio of the spin carried by the protons at zero momentum is given by $⟨S_p^Na⟩/⟨S_p^I⟩∼0.7$ [ref] .","intent_p":0.94,"contests_p":null},{"arxiv_id":"1907.07682","title":"Direct Detection of Spin-(In)dependent Nuclear Scattering of Sub-GeV Dark Matter Using Molecular Excitations","url":"/paper/1907.07682","section":"Spin-Dependent Nuclear Recoils","sentence":"The values of $⟨S_P ⟩$ and $⟨S_N ⟩$ have been calculated in the odd group approximation [ref] .","intent_p":0.84,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":8,"sentences":8,"quotes":[{"arxiv_id":"1108.4337","title":"On the formalism and upper limits for spin-dependent cross sections in dark matter elastic scattering with nuclei","url":"/paper/1108.4337","section":"Structure functions and “form factors”","sentence":"Detailed nuclear shell-model calculations of the spin matrix elements in the zero momentum transfer limit (ZMTL), i.e. point-like nucleus, and of the SSF that account for the momentum transfer dependence response, have been carried out for many nuclei employed in actual experiments, see [ref] for reviews.","intent_p":0.94,"contests_p":null},{"arxiv_id":"1306.1858","title":"Lowering the Threshold in the DAMA Dark Matter Search","url":"/paper/1306.1858","section":"Dark Matter Direct Detection","sentence":"A description of form factors can be found in Refs. [ref] (SI) and Refs. [ref] (SD).","intent_p":0.96,"contests_p":null},{"arxiv_id":"1804.01231","title":"Dark Matter implications of DAMA/LIBRA-phase2 results","url":"/paper/1804.01231","section":"Annual Modulation","sentence":"The nuclear form factor $F(q)$ accounts for the finite size of the nucleus, see e.g. [ref] for the form factor in the SI case and [ref] for the SD case.","intent_p":0.82,"contests_p":null},{"arxiv_id":"1204.1339","title":"Dark Matter collisions with the Human Body","url":"/paper/1204.1339","section":"Introduction","sentence":"More detailed discussions of dark matter scattering kinematics, cross-sections, and form factors can be found in Refs. [ref] ; other reviews can be found in Refs. [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1011.6108","title":"A scheme for the extraction of WIMP-nucleon scattering cross sections from total event rates","url":"/paper/1011.6108","section":"Introduction","sentence":"One of the most studied WIMP candidate is the lightest neutralino in the minimal supersymmetric standard model (MSSM) with $R$-parity conservation [ref] .","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":31},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"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/hep-ph/0406218"}}