{"paper":{"title":"Cosmic-ray Antinuclei as Messengers of New Physics: Status and Outlook for the New Decade","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Datta, A. Lowell, A. Oliva, A. Shukla, A. Stoessl, C. Evoli, C. Gerrity, C. Hailey, D. Gomez Coral, D. Hooper, D. Wright, E. Ferronato Bueno, E. Vannuccini, F. Donato, F. Nozzoli, F. Rogers, G. Osteria, G. Zampa, H. Fuke, I.V. Moskalenko, J. Ryan, J. Tjemsland, K.C.Y. Ng, K. Perez, K. Sakai, L. Fabbietti, L. Fabris, L. Serksnyte, M. Boezio, M. Cui, M. Kachelriess, M. Korsmeier, M. Kozai, M. Manghisoni, M. Naskret, M. Vecchi, M.W. Winkler, M. Xiao, N. Fornengo, N. Li, N. Saffold, P. Salati, P. von Doetinchem, P. Zuccon, R.A. Ong, R. Bird, R. Lea, R. Munini, S. Baker, S. Barwick, S.E. Boggs, S. Profumo, S. Quinn, S. Schael, T. Aramaki, T. Nelson, T. Pierog, T. Poeschl, T. Yoshida, V. Poulin, V.Re, W. Xu","submitted_at":"2020-02-11T01:41:13Z","abstract_excerpt":"The precise measurement of cosmic-ray antinuclei serves as an important means for identifying the nature of dark matter and other new astrophysical phenomena, and could be used with other cosmic-ray species to understand cosmic-ray production and propagation in the Galaxy. For instance, low-energy antideuterons would provide a \"smoking gun\" signature of dark matter annihilation or decay, essentially free of astrophysical background. Studies in recent years have emphasized that models for cosmic-ray antideuterons must be considered together with the abundant cosmic antiprotons and any potential"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2002.04163","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2002.04163/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}