{"arxiv_id":"1201.2699","incoming":{"papers":16,"sentences":28,"groups":[{"kind":"comparison","label":"Compares with it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1205.0673","title":"Upper Bounds on Asymmetric Dark Matter Self Annihilation Cross Sections","url":"/paper/1205.0673","section":"Boltzmann equations for asymmetric dark matter","sentence":"which is close to the estimated bound on gaugino masses given in [ref] from the same argument.","intent_p":0.94,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1611.04693","title":"Asymmetric Dark Matter Models in SO(10)","url":"/paper/1611.04693","section":"Hypercharged asymmetric dark matter","sentence":"This incompatibility disfavors most of the hypercharged asymmetric dark matter candidates [ref] .","intent_p":0.99,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":5,"sentences":6,"quotes":[{"arxiv_id":"1202.0283","title":"Oscillating Asymmetric Dark Matter","url":"/paper/1202.0283","section":"Introduction","sentence":"This effect has been discussed within the context of specific models [ref] , and emphasized more generally in Refs. [ref] .","intent_p":0.86,"contests_p":null},{"arxiv_id":"1205.0673","title":"Upper Bounds on Asymmetric Dark Matter Self Annihilation Cross Sections","url":"/paper/1205.0673","section":"Boltzmann equations for asymmetric dark matter","sentence":"Higgsinos $h̃_u$, $h̃_d$ with masses $m ∼200-1000$ GeV as ADM were proposed recently in [ref] .","intent_p":0.81,"contests_p":null},{"arxiv_id":"1210.0094","title":"Phenomenology of WIMPy baryogenesis models","url":"/paper/1210.0094","section":"Introduction","sentence":"This intriguing possibility has been vastly explored in the literature, mostly by invoking asymmetric DM (ADM) scenarios [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"1212.0011","title":"Higgsino Dark Matter and the Cosmological Gravitino Problem","url":"/paper/1212.0011","section":"Introduction","sentence":"It is this cosmological motivation, relating to the moduli problem, that will be discussed in detail in the present article [We note that Higgsino dark matter has cosmological motivations other than the ones considered here, for example from baryogenesis [ref] .].","intent_p":0.94,"contests_p":null},{"arxiv_id":"1407.0017","title":"Dark matter production in the early Universe: beyond the thermal WIMP paradigm","url":"/paper/1407.0017","section":"Asymmetric dark matter (ADM)","sentence":"Some examples of ADM include technibaryons [ref] , mirror dark matter [ref] , scalar neutrinos [ref] , pure higgsinos [ref] and others.","intent_p":0.91,"contests_p":null}]}],"unlabelled_sentences":20},"outgoing":{"papers":20,"sentences":22,"groups":[{"kind":"method_or_tool","label":"Uses the method or tool of","papers":1,"sentences":1,"quotes":[{"arxiv_id":"0807.2283","title":"The Effect of the Sparticle Mass Spectrum on the Conversion of B-L to B","url":"/paper/0807.2283","section":"Introduction","sentence":"We follow the derivation of Refs. [ref] .","intent_p":1.0,"contests_p":null}]},{"kind":"comparison","label":"Compares with","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1109.2164","title":"Regenerating a Symmetry in Asymmetric Dark Matter","url":"/paper/1109.2164","section":"Introduction","sentence":"Our equations are consistent with those of Ref. [ref] which deals with closely related issues (see also [ref] ).","intent_p":0.87,"contests_p":null},{"arxiv_id":"1110.3809","title":"Consequences of DM/antiDM Oscillations for Asymmetric WIMP Dark Matter","url":"/paper/1110.3809","section":"Introduction","sentence":"Our equations are consistent with those of Ref. [ref] which deals with closely related issues (see also [ref] ).","intent_p":0.87,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"0802.2962","title":"Leptogenesis","url":"/paper/0802.2962","section":"Introduction","sentence":"Perhaps the most plausible one is via leptogenesis (for a review, see [ref] ).","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":18},"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/1201.2699"}}