{"arxiv_id":"hep-ph/0308015","incoming":{"papers":33,"sentences":37,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":2,"quotes":[{"arxiv_id":"1005.4840","title":"Non-standard primordial fluctuations and nongaussianity in string inflation","url":"/paper/1005.4840","section":"Dynamics of the curvaton field $χ_1$","sentence":"In this work, we follow the prescription of [ref] , but our approach can be adapted to different possibilities.","intent_p":0.99,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":20,"sentences":21,"quotes":[{"arxiv_id":"2606.28296","title":"Memoirs of the curvaton: non-perturbative non-Gaussianity and supermassive primordial black holes","url":"/paper/2606.28296","section":"Introduction","sentence":"During the last two decades, several studies have highlighted how a light spectator field, known as the curvaton, can generate large-amplitude perturbations after inflation [ref] , which, under suitable conditions, are capable of producing PBHs [ref] and SIGWs.","intent_p":0.93,"contests_p":null},{"arxiv_id":"0807.0382","title":"Parametric Decay of the Curvaton","url":"/paper/0807.0382","section":"The inflationary period","sentence":"Since the curvaton is very light, its equation of motion is approximatively given by $3H_*σ̇≃-m_σ^2σ$ (for a discussion of curvaton dynamics in various potentials, see [ref] ).","intent_p":0.9,"contests_p":null},{"arxiv_id":"0912.3394","title":"Curvaton decay into relativistic matter","url":"/paper/0912.3394","section":"Introduction","sentence":"A well motivated alternative to the simplest inflationary scenario is the curvaton mechanism [ref] in which the perturbations are generated by a second scalar field, called the curvaton, which stays subdominant during inflation and the actual expansion of space is still driven by the inflaton.","intent_p":0.8,"contests_p":null},{"arxiv_id":"1502.07339","title":"Scale-dependent non-Gaussianity and the CMB Power Asymmetry","url":"/paper/1502.07339","section":"The self–interacting curvaton scenario","sentence":"The phenomenology of this model has been extensively studied in previous work, see e.g. [ref] , where it was found that observable quantities (such as $$) can depart substantially from the standard quadratic curvaton prediction due to self–interactions.","intent_p":0.9,"contests_p":null},{"arxiv_id":"0912.4657","title":"Non-Gaussian Fingerprints of Self-Interacting Curvaton","url":"/paper/0912.4657","section":"Introduction","sentence":"Predictions of the curvaton scenario depend crucially on the form of the curvaton potential [ref] (and the background evolution [ref] ).","intent_p":0.85,"contests_p":null}]}],"unlabelled_sentences":14},"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/0308015"}}