{"arxiv_id":"hep-ph/0312002","incoming":{"papers":38,"sentences":54,"groups":[{"kind":"comparison","label":"Compares with it","papers":1,"sentences":3,"quotes":[{"arxiv_id":"1409.1734","title":"Disformal Theories of Gravity: From the Solar System to Cosmology","url":"/paper/1409.1734","section":"Introduction","sentence":"Comparing our results with those of [ref] , who study the quantum loop corrections arising from the disformal coupling $T^∂_μϕ∂_νϕ/ℳ^4$, we find that $ℳ𝒪(eV)$ whereas they find $ℳ𝒪(10^2GeV)$ using mono-photon searches at the LHC.","intent_p":0.99,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":24,"sentences":25,"quotes":[{"arxiv_id":"1909.11756","title":"Cosmological attractors to general relativity and spontaneous scalarization with disformal coupling","url":"/paper/1909.11756","section":"Introduction","sentence":"They have been studied mainly in cosmology [ref] and have also been shown to allow for spontaneous scalarization of NSs [ref] .","intent_p":0.93,"contests_p":null},{"arxiv_id":"1507.00568","title":"Solar System Constraints on Disformal Gravity Theories","url":"/paper/1507.00568","section":"Introduction","sentence":"The term proportional to $D$ is known as the disformal coupling and, in contrast to the first term—the conformal coupling—it has only recently begun to be studied in detail [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"1510.01650","title":"Disformally coupled inflation","url":"/paper/1510.01650","section":"Introduction","sentence":"Kaloper [ref] proposed a model with a disformal coupling of a massless inflaton to the Standard model, and found that such coupling could be well constrained by collider experiments such as the LHC, as confirmed by more recent studies [ref] , though these constraints can be avoided if the disformal coupling is suppressed in the Standard model sector after reheating.","intent_p":0.91,"contests_p":null},{"arxiv_id":"1310.7597","title":"How Fabulous Is Fab 5 Cosmology?","url":"/paper/1310.7597","section":"Soundness and Naturalness","sentence":"(For more on disformal theories, see e.g. [ref] .) The field has no potential term so the theory is manifestly shift symmetric.","intent_p":1.0,"contests_p":null},{"arxiv_id":"1206.1809","title":"Shining Light on Modifications of Gravity","url":"/paper/1206.1809","section":"Introduction","sentence":"The metric that is induced on the brane is [equation] * Disformal couplings arise in theories in which Lorentz invariance is broken spontaneously on a non-trivial background [ref] . * The effects of including disformal couplings in chameleon theories were considered in [ref] . * Scalar fields with disformal couplings have been used to give rise to unusual forms of cosmic acceleration, called disformal inflation [ref] in the early universe and disformal quintessence [ref] in the late universe.","intent_p":0.95,"contests_p":null}]}],"unlabelled_sentences":26},"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/0312002"}}