{"arxiv_id":"1202.0698","incoming":{"papers":11,"sentences":14,"groups":[{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1306.0911","title":"Kasner solutions, climbing scalars and big-bang singularity","url":"/paper/1306.0911","section":"Conclusions","sentence":"Indeed, recent results in [ref] indicate that a climbing phase would lead to a dampening of the power spectrum on large scales and oscillations superimposed on it that fit relatively well the Planck 2013 data [ref] .","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":4,"sentences":4,"quotes":[{"arxiv_id":"1906.03942","title":"Unique contributions to the scalar bispectrum in `just enough inflation'","url":"/paper/1906.03942","section":"Introduction","sentence":"A model that has drawn recent attention in the context of suppressing power on large scales involves a scalar field which begins its journey down the inflationary potential with the largest initial velocity possible (for the original discussion, see Ref. [ref] ; for recent discussions, see Refs. [ref] ).","intent_p":0.85,"contests_p":null},{"arxiv_id":"1211.1707","title":"Inflection Points and the Power Spectrum","url":"/paper/1211.1707","section":"Introduction","sentence":"Possible origins for these effects have been studied previously [ref] , but generally in the context of the minimal “just enough” inflation.","intent_p":0.93,"contests_p":null},{"arxiv_id":"1504.03682","title":"Signatures of the Very Early Universe: Inflation, Spatial Curvature and Large Scale Anomalies","url":"/paper/1504.03682","section":"Introduction","sentence":"However, there is long-standing interest in “Just Enough\" inflation (e.g. Refs [ref] ).","intent_p":0.82,"contests_p":null},{"arxiv_id":"2402.18494","title":"Open EFT treatment of Inflation with Thermal Initial Conditions","url":"/paper/2402.18494","section":"Introduction","sentence":"There have been several attempts to resolve the low-$ℓ$ problem, including topological defects of cosmic strings in pre-slow-roll era [ref] , a contracting phase in pre-slow-roll era [ref] , just-enough inflation [ref] , punctuated inflation [ref] , cosmic variance [ref] , and resonant superstring excitations during inflation [ref] .","intent_p":0.81,"contests_p":null}]}],"unlabelled_sentences":9},"outgoing":{"papers":13,"sentences":32,"groups":[{"kind":"extends","label":"Builds on","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1111.7131","title":"Predictions of just-enough inflation","url":"/paper/1111.7131","section":"introduction","sentence":"Following previous works in which a modification of the chaotic inflation scenario [ref] is proposed to quantify the predictions of the $λϕ^4$ potential [ref] , in this work the idea is further applied to the $m^2ϕ^2$ potential and a hybrid inflation potential during the stage when there is effectively a single field leading the dynamics.","intent_p":0.99,"contests_p":null}]},{"kind":"method_or_tool","label":"Uses the method or tool 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.","intent_p":0.97,"contests_p":null}]},{"kind":"comparison","label":"Compares with","papers":2,"sentences":4,"quotes":[{"arxiv_id":"1111.7131","title":"Predictions of just-enough inflation","url":"/paper/1111.7131","section":"results","sentence":"The values of $ΔAIC$ for both potentials here are smaller than those for the $λϕ^4$ potential as seen in [ref] , the difference for the $m^2ϕ^2$ potential is the smallest of the three cases.","intent_p":1.0,"contests_p":null},{"arxiv_id":"astro-ph/0303636","title":"Suppressing the lower Multipoles in the CMB Anisotropies","url":"/paper/astro-ph/0303636","section":"introduction","sentence":"The predictions and results for this case are in accordance to those found in [ref] , applied to the scenario already mentioned in [ref] , in which the form of the power spectrum does not show a significant dependence on the choice of initial conditions.","intent_p":0.86,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites as 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.","intent_p":0.8,"contests_p":null},{"arxiv_id":"0804.2387","title":"The CMB Quadrupole depression produced by early fast-roll inflation: MCMC analysis of WMAP and SDSS data","url":"/paper/0804.2387","section":"Low Multipoles","sentence":"An early epoch of kinetic energy domination has been proposed as an explanation for the smaller than expected power of the low multipoles of the CMB anisotropies [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] .","intent_p":0.8,"contests_p":null},{"arxiv_id":"0808.3767","title":"No large-angle correlations on the non-Galactic microwave sky","url":"/paper/0808.3767","section":"Low Multipoles","sentence":"An early epoch of kinetic energy domination has been proposed as an explanation for the smaller than expected power of the low multipoles of the CMB anisotropies [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] .","intent_p":0.8,"contests_p":null},{"arxiv_id":"1111.7131","title":"Predictions of just-enough inflation","url":"/paper/1111.7131","section":"Low Multipoles","sentence":"An early epoch of kinetic energy domination has been proposed as an explanation for the smaller than expected power of the low multipoles of the CMB anisotropies [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] .","intent_p":0.8,"contests_p":null},{"arxiv_id":"astro-ph/0303636","title":"Suppressing the lower Multipoles in the CMB Anisotropies","url":"/paper/astro-ph/0303636","section":"Low Multipoles","sentence":"An early epoch of kinetic energy domination has been proposed as an explanation for the smaller than expected power of the low multipoles of the CMB anisotropies [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] , [ref] .","intent_p":0.8,"contests_p":null}]}],"unlabelled_sentences":17},"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/1202.0698"}}