{"arxiv_id":"1608.03386","incoming":{"papers":3,"sentences":3,"groups":[{"kind":"background","label":"Cites it as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2408.16043","title":"Gravitino Thermal Production, Dark Matter, and Reheating of the Universe","url":"/paper/2408.16043","section":"Introduction","sentence":"In the context of the gauge mediated supersymmetry breaking scenario, a different production mechanism is used [ref] [See also [ref] for various works on gravitino production and DM.].","intent_p":0.85,"contests_p":null},{"arxiv_id":"1708.02830","title":"Supergravity Models with 50-100 TeV Scalars, SUSY Discovery at the LHC and Gravitino Decay Constraints","url":"/paper/1708.02830","section":"The Gravitino Decay Constraints","sentence":"A brief list of these include [ref] .","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":1},"outgoing":{"papers":21,"sentences":28,"groups":[{"kind":"data_used","label":"Uses data or values from","papers":2,"sentences":2,"quotes":[{"arxiv_id":"0907.5003","title":"Nucleosynthesis Constraints on a Massive Gravitino in Neutralino Dark Matter Scenarios","url":"/paper/0907.5003","section":"Out of equilibrium production of gravitinos","sentence":"In order that the abundance lie within the cosmological bound of order $10^-14$ as given in Ref. [ref] , $T_reh$ should be less than $4×10^4$.","intent_p":0.92,"contests_p":null},{"arxiv_id":"hep-ph/0612291","title":"Constraints on the Reheating Temperature in Gravitino Dark Matter Scenarios","url":"/paper/hep-ph/0612291","section":"Gravitino production","sentence":"where $i=1,2,3$ refers to the three gauge groups $U(1)_Y, SU(2)_L$ and $SU(3)_c$ respectively, $g_i(T)$ are the gauge coupling constants (evaluated at the most relevant temperature), and $c_1,2,3=11, 27,72$ and $k_1,2,3=1.266, 1.312, 1.271$ are constants associated with the gauge groups (see Table 1 of Ref. [ref] ).","intent_p":0.91,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":14,"sentences":16,"quotes":[{"arxiv_id":"astro-ph/0408426","title":"Big-Bang Nucleosynthesis and Hadronic Decay of Long-Lived Massive Particles","url":"/paper/astro-ph/0408426","section":"Introduction","sentence":"Gravitinos are produced in the early Universe either in the radiation dominated Universe after reheating [ref] , or during standard (perturbative) reheating [ref] , by the scattering of thermalised inflaton decay products.","intent_p":0.96,"contests_p":null},{"arxiv_id":"hep-ph/9911302","title":"Thermal and Non-Thermal Production of Gravitinos in the Early Universe","url":"/paper/hep-ph/9911302","section":"Introduction","sentence":"Gravitinos are produced in the early Universe either in the radiation dominated Universe after reheating [ref] , or during standard (perturbative) reheating [ref] , by the scattering of thermalised inflaton decay products.","intent_p":0.96,"contests_p":null},{"arxiv_id":"0811.1866","title":"Perturbative Reheating and Gravitino Production in Inflationary Models","url":"/paper/0811.1866","section":"Introduction","sentence":"Gravitinos are produced in the early Universe either in the radiation dominated Universe after reheating [ref] , or during standard (perturbative) reheating [ref] , by the scattering of thermalised inflaton decay products.","intent_p":0.96,"contests_p":null},{"arxiv_id":"hep-ph/0612291","title":"Constraints on the Reheating Temperature in Gravitino Dark Matter Scenarios","url":"/paper/hep-ph/0612291","section":"Introduction","sentence":"Gravitinos are produced in the early Universe either in the radiation dominated Universe after reheating [ref] , or during standard (perturbative) reheating [ref] , by the scattering of thermalised inflaton decay products.","intent_p":0.96,"contests_p":null},{"arxiv_id":"hep-ph/0107212","title":"The Inflatino Problem in Supergravity Inflationary Models","url":"/paper/hep-ph/0107212","section":"Introduction","sentence":"Gravitinos can also be produced during preheating [ref] or via direct inflaton decay [ref] , or during and after inflation in warm inflation scenarios [ref] .","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":10},"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/1608.03386"}}