{"arxiv_id":"hep-ph/9710415","incoming":{"papers":10,"sentences":17,"groups":[{"kind":"comparison","label":"Compares with it","papers":2,"sentences":3,"quotes":[{"arxiv_id":"2309.00672","title":"Sphaleron freeze-in baryogenesis with gravitational waves from the QCD transition","url":"/paper/2309.00672","section":"Introduction","sentence":"We find that the lepton asymmetries required to produce the observed baryon asymmetry are about an order of magnitude smaller than previous estimates based on a perturbative effective potential [ref] .","intent_p":0.93,"contests_p":null},{"arxiv_id":"2407.17549","title":"Baryogenesis and first-order QCD transition with gravitational waves from a large lepton asymmetry","url":"/paper/2407.17549","section":"Sphaleron freeze-in baryogenesis and generation of a large lepton asymmetry","sentence":"Remarkably, our approach predicts a reduction by an order of magnitude in the required primordial lepton asymmetry necessary for successful baryogenesis compared to prior findings in the literature, such as Refs. [ref] .","intent_p":0.98,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":8,"sentences":8,"quotes":[{"arxiv_id":"2501.13153","title":"Neutrinophilic $\\mathbf{\\Lambda}$CDM Extension for EMPRESS, DESI and Hubble Tension","url":"/paper/2501.13153","section":"Introduction","sentence":"Despite the sphaleron process in the early universe [ref] , various models can generate a PNA $η_ν$ that is much larger than the baryon asymmetry of the universe $η_B ≡n_B/n_γ ∼𝒪(10^-10)$ [ref] .","intent_p":0.84,"contests_p":null},{"arxiv_id":"2309.00672","title":"Sphaleron freeze-in baryogenesis with gravitational waves from the QCD transition","url":"/paper/2309.00672","section":"Introduction","sentence":"The various existing studies in the literature [ref] employ the perturbative effective potential at finite temperature and chemical potential.","intent_p":0.82,"contests_p":null},{"arxiv_id":"2407.17549","title":"Baryogenesis and first-order QCD transition with gravitational waves from a large lepton asymmetry","url":"/paper/2407.17549","section":"The perturbative approach and motivation to go beyond","sentence":"Large lepton asymmetry as an explanation of the absence of topological defects has been discussed in [ref] , while in [ref] a large lepton asymmetry has been used to explain the observed baryon asymmetry of the Universe.","intent_p":0.93,"contests_p":null},{"arxiv_id":"2302.07002","title":"Gravitational capture of magnetic monopoles by primordial black holes in the early universe","url":"/paper/2302.07002","section":"Introduction","sentence":"Other solutions to the monopole problem include inverse symmetry breaking or symmetry nonrestoration effect in finite-temperature field theory [ref] , eliminating the monopoles by domain walls which subsequently decay or get destroyed [ref] , entropy production effects [ref] , and gravitational capture by primordial black holes (PBHs) which evaporate prior to BBN [ref] .","intent_p":0.89,"contests_p":null},{"arxiv_id":"2210.05680","title":"Electroweak Asymmetric Early Universe via a Scalar Condensate","url":"/paper/2210.05680","section":"Introduction","sentence":"The possibility of the higgs field acquiring a nonzero vacuum expectation value (vev) in the early universe has wide reaching consequences, some of which have been explored in [ref] .","intent_p":0.86,"contests_p":null}]}],"unlabelled_sentences":6},"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/9710415"}}