{"arxiv_id":"1210.7975","incoming":{"papers":15,"sentences":15,"groups":[{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1312.2961","title":"Delaying the waterfall transition in warm hybrid inflation","url":"/paper/1312.2961","section":"Warm regime","sentence":"In this example, a large number of waterfall fields was considered, which is generically required in order to keep the system in the warm regime with the form of the dissipation coefficient considered, as observed in [ref] .","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2012.03988","title":"Warm Inflation, Neutrinos and Dark matter: a minimal extension of the Standard Model","url":"/paper/2012.03988","section":"Introduction","sentence":"This scenario constitutes the first successful implementation of warm inflation within a concrete extension of the SM, building upon a large 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amplitude $𝒫_ℛ=(2.43±0.11)×10^-9$ and a spectral index $n_s =0.967±0.014$ [ref] to determine $V_0$ and $ϕ_*$.","intent_p":1.0,"contests_p":null}]},{"kind":"comparison","label":"Compares with","papers":1,"sentences":1,"quotes":[{"arxiv_id":"0902.0521","title":"Warm inflation model building","url":"/paper/0902.0521","section":"Summary and future prospects","sentence":"The minimum value of $C_ϕ≳10^6$ obtained for $g_*=100$ is of the same order as that obtained for other forms of the inflaton potential, such as monomial or hybrid models [ref] , which implies large couplings and field multiplicities, so one may ask whether there is any gain from the model building perspective in trading a large fine-tuning in the parameters of the potential for large couplings and a large number of fields.","intent_p":0.99,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":10,"sentences":11,"quotes":[{"arxiv_id":"0808.0261","title":"On the consistency of warm 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expansion from the adiabatic motion of the inflaton field, which may be analyzed within the framework of linear response theory.","intent_p":0.93,"contests_p":null},{"arxiv_id":"hep-ph/0308211","title":"Absence of isentropic expansion in various inflation models","url":"/paper/hep-ph/0308211","section":"Introduction","sentence":"Most scenarios considered in the literature so far in the context of quantum field theory [ref] , as well as phenomenological models [ref] consider the case where a nearly-thermal bath of radiation is produced concurrently with accelerated expansion from the adiabatic motion of the inflaton field, which may be analyzed within the framework of linear response theory.","intent_p":0.93,"contests_p":null}]}],"unlabelled_sentences":36},"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. 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