{"arxiv_id":"astro-ph/0312605","incoming":{"papers":32,"sentences":46,"groups":[{"kind":"background","label":"Cites it as background","papers":16,"sentences":16,"quotes":[{"arxiv_id":"1109.3725","title":"Neutron Oscillations to Parallel World: Earlier End to the Cosmic Ray Spectrum?","url":"/paper/1109.3725","section":"Introduction","sentence":"To conclude, concept of parallel/mirror sector with exactly the same microphysics as the ordinary particle sector provides an interesting possibility for dark matter [ref] and a peculiar way for its testing via oscillation phenomena of ordinary neutral particles in their mass degenerate mirror twins.","intent_p":0.86,"contests_p":null},{"arxiv_id":"1310.8642","title":"Snowmass-2013 Cosmic Frontier 3 (CF3) Working Group Summary: Non-WIMP dark matter","url":"/paper/1310.8642","section":"Mirror dark matter","sentence":"To see why this answer is reasonable, one has to understand mirror dark matter cosmology [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"2409.16095","title":"Low-scale Mirror Standard Model Dark Matter and its Detection via Gravitational Waves and the Guitar Nebula","url":"/paper/2409.16095","section":"Introduction","sentence":"Regarding DM, there is a not so well popular class of DM theories, which have incredibly interesting phenomenological features, the mirror DM theories firstly introduced in [ref] and further developed in Refs. [ref] see also Refs. [ref] for further applications.","intent_p":0.98,"contests_p":null},{"arxiv_id":"2110.04317","title":"Mirror Twin Higgs Cosmology: Constraints and a Possible Resolution to the $H_0$ and $S_8$ Tensions","url":"/paper/2110.04317","section":"Constraints from CMB Measurements","sentence":"Furthermore, we predicted that these effects would show up in two forms: an overall suppression of the matter power spectrum, and an oscillatory pattern (in $k$-space) for the $k$-modes that enter the horizon before twin recombination.[For earlier work on LSS in the context of mirror models, see [ref] .","intent_p":0.94,"contests_p":null},{"arxiv_id":"0904.3609","title":"Notes on Hidden Mirror World","url":"/paper/0904.3609","section":"Dark Matter Candidates and Mirror Matter","sentence":"After [ref] about 300 papers have been published (among them e.g. Z.Berezhiani, R.Foot were very active, e.g. [ref] ), an extensive review of the literature on the subject is written by Okun [ref] .","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":30},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[{"relation":"same_result","label":"States the same result","papers":[{"arxiv_id":"astro-ph/0409629","url":"/paper/astro-ph/0409629","title":"Structure formation, CMB and LSS in a mirror dark matter scenario","main_claim":"We show mirror models for CMB and LSS power spectra and compare them with observations, obtaining bounds on the mirror parameter space.","p":1.0}]}],"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/astro-ph/0312605"}}