{"arxiv_id":"2108.02383","incoming":{"papers":9,"sentences":10,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2312.10414","title":"Baryogenesis in $R^2$-Higgs Inflation: the Gravitational Connection","url":"/paper/2312.10414","section":"Inflationary Dynamics in the Covariant Formalism","sentence":"We now study the inflationary dynamics of our two-field scenario with the non-canonical kinetic term (i.e. with a nontrivial field-space manifold) following the covariant formalism discussed in Refs. [ref] (see also Refs. [ref] ).","intent_p":0.98,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":4,"sentences":4,"quotes":[{"arxiv_id":"2205.14813","title":"The Inflaton that Could : Primordial Black Holes and Second Order Gravitational Waves from Tachyonic Instability induced in Higgs-$R^2$ Inflation","url":"/paper/2205.14813","section":"Introduction","sentence":"Among many inflationary models, Higgs inflation [ref] and its extensions [ref] gain immense interest as it incorporates the Standard Model scalar with a nonminimal coupling to gravity, and it provides the best fit to current cosmic microwave background (CMB) observations.","intent_p":0.84,"contests_p":null},{"arxiv_id":"2404.02492","title":"Enhanced Curvature Perturbation and Primordial Black Hole Formation in Two-stage Inflation with a break","url":"/paper/2404.02492","section":"Introduction","sentence":"There are a number of proposed mechanisms to enhance the primordial curvature perturbations during inflation, for instance, single-field inflation with a non-slow-roll stage [ref] , multi-field inflation [ref] , modify gravity [ref] , curvaton scenario [ref] , parametric resonance [ref] , etc.","intent_p":0.99,"contests_p":null},{"arxiv_id":"2302.05866","title":"Nonminimally Assisted Inflation: A General Analysis","url":"/paper/2302.05866","section":"Model","sentence":"See, e.g., Refs. [ref] for such works.","intent_p":1.0,"contests_p":null},{"arxiv_id":"2406.09045","title":"Pseudo-Nambu-Goldstone Boson Production from Inflaton Coupling during Reheating","url":"/paper/2406.09045","section":"Application: PQ Inflation with Large Non-minimal Coupling","sentence":"Many works are done in the Higgs inflation context [ref] .","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":5},"outgoing":{"papers":3,"sentences":3,"groups":[{"kind":"contests","label":"Contests","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2105.02143","title":"Inflation, electroweak phase transition, and Higgs searches at the LHC in the two-Higgs-doublet model","url":"/paper/2105.02143","section":"Introduction","sentence":"The work here also remedies the shortcomings of Ref. [ref] where inflationary dynamics was also under scrutiny due to the unitarity violation by the required large nonminimal couplings $𝒪(10^4 - 6×10^4)$ as in the SM [ See also Refs. [ref] for discussions on inflation in the 2HDM.].","intent_p":0.83,"contests_p":0.85}]},{"kind":"data_used","label":"Uses data or values from","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2110.00483","title":null,"url":"/paper/2110.00483","section":"Background Dynamics and Power Spectrum","sentence":"By including the BICEP/Keck 2018 data, the constraint became tighter as $r< 0.036$ [ref] .","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":1},"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/2108.02383"}}