{"arxiv_id":"1403.1561","incoming":{"papers":1,"sentences":1,"groups":[],"unlabelled_sentences":1},"outgoing":{"papers":25,"sentences":65,"groups":[{"kind":"method_or_tool","label":"Uses the method or tool of","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1305.0237","title":"micrOMEGAs3.1 : a program for calculating dark matter observables","url":"/paper/1305.0237","section":"Selection of parameter sets","sentence":"In the calculation, we use MicrOMEGAs [ref] included in NMSSMTools.","intent_p":1.0,"contests_p":null}]},{"kind":"data_used","label":"Uses data or values from","papers":10,"sentences":16,"quotes":[{"arxiv_id":"0805.3389","title":"Big-bang nucleosynthesis and the relic abundance of dark matter in a stau-neutralino coannihilation scenario","url":"/paper/0805.3389","section":"Exotic BBN reactions","sentence":"The timescale to form bound state ($^7$Be $l̃^-$) is $O(10^3)$ s [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"astro-ph/0510636","title":"Lithium isotopic abundances in metal-poor halo stars","url":"/paper/astro-ph/0510636","section":"Constraints from BBN","sentence":"We adopt following observational bounds on light element abundances: the lithium 7 to hydrogen ratio $Log_10(^7Li/H) = -9.63 ±0.06$ [ref] , the lithium 6 to lithium 7 ratio $^6$Li/$^7$Li $= 0.046 ±0.022$ [ref] , the deuterium to hydrogen ratio D/H = $(2.80 ±0.20) ×10^-5$ [ref] , and the helium 3 to deuterium ratio $^3$He/D $<$ 0.87 + 0.27 [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1105.1431","title":"Big-bang nucleosynthesis with a long-lived charged massive particle including $^4$He spallation processes","url":"/paper/1105.1431","section":"Introduction","sentence":"The standard calculation predicts the ratio of abundance $Log_10(^7Li/H)$ to be $-9.35±0.06$ [ref] , while the observation indicates $-9.63 ±0.06$ [ref] .","intent_p":0.87,"contests_p":null},{"arxiv_id":"hep-ph/0702274","title":"Stau-catalyzed $^6$Li Production in Big-Bang Nucleosynthesis","url":"/paper/hep-ph/0702274","section":"BBN results at the benchmark points","sentence":"The horizontal black-dashed line represents the timescale of the catalyzed fusion process [ref] [ref] at the temperature $T=5$ keV ($5×10^4$ s) when ($^4$He $l̃^-$) is formed.","intent_p":0.81,"contests_p":null},{"arxiv_id":"1303.5076","title":"Planck 2013 results. XVI. Cosmological parameters","url":"/paper/1303.5076","section":"Selection of parameter sets","sentence":"The latest result for observed abundance of dark matter is reported by the Planck Collaboration [equation] at the $3σ$ level [ref] , and we apply this result as a constraint.","intent_p":1.0,"contests_p":null}]},{"kind":"comparison","label":"Compares with","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1105.1431","title":"Big-bang nucleosynthesis with a long-lived charged massive particle including $^4$He spallation processes","url":"/paper/1105.1431","section":"BBN results at the benchmark points","sentence":"Indeed, the results at BL-1, BL-2, and BL-3 are almost same as the result in the MSSM, Fig. 3 in Ref. [ref] , where the same values for $c_e, m_χ̃^0_1, sinθ_f$ and CP-violating phase are used.","intent_p":1.0,"contests_p":null},{"arxiv_id":"1208.5533","title":"Allowed slepton intergenerational mixing in light of light element abundances","url":"/paper/1208.5533","section":"BBN results at the benchmark points","sentence":"This result is similar to that in the MSSM, Fig. 4 (middle panel) in Ref. [ref] , where same values for $c_e, m_χ̃^0_1, sinθ_f$ and CP-violating phase are used.","intent_p":1.0,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":5,"sentences":5,"quotes":[{"arxiv_id":"1105.1431","title":"Big-bang nucleosynthesis with a long-lived charged massive particle including $^4$He spallation processes","url":"/paper/1105.1431","section":"Exotic BBN reactions","sentence":"The last one is the $^4$He spallation processes [ref] :","intent_p":0.81,"contests_p":null},{"arxiv_id":"1303.5076","title":"Planck 2013 results. XVI. Cosmological parameters","url":"/paper/1303.5076","section":"Introduction","sentence":"Among such questions is the nature of dark matter; it became a compelling question during this decade after the precise observations of the universe reported their results [ref] .","intent_p":0.91,"contests_p":null},{"arxiv_id":"1212.5225","title":"Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results","url":"/paper/1212.5225","section":"Introduction","sentence":"Among such questions is the nature of dark matter; it became a compelling question during this decade after the precise observations of the universe reported their results [ref] .","intent_p":0.91,"contests_p":null},{"arxiv_id":"1207.7214","title":"Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC","url":"/paper/1207.7214","section":"Introduction","sentence":"The recent discovery of the Higgs particle finally crowned the accumulation of successes [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1207.7235","title":"Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC","url":"/paper/1207.7235","section":"Introduction","sentence":"The recent discovery of the Higgs particle finally crowned the accumulation of successes [ref] .","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":41},"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/1403.1561"}}