{"paper":{"title":"Cosmology Intertwined III: $f \\sigma_8$ and $S_8$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Adam G. Riess, Adri\\`a G\\'omez-Valent, Agn\\`es Fert\\'e, Alan Heavens, Alessandra Silvestri, Alessandro Melchiorri, Alessio Notari, Andronikos Paliathanasis, Angela Chen, Anil K. Yadav, Anjan A. Sen, Ankan Mukherjee, Anowar J. Shajib, Anton Chudaykin, Antonella Palmese, Arindam Mazumdar, Arman Shafieloo, Benjamin D. Wandelt, Carsten van de Bruck, Celia Escamilla-Rivera, Cristian Moreno-Pulido, Daniela Paoletti, Daniel Holz, David Camarena, David F. Mota, Deng Wang, Dragan Huterer, Elena Giusarma, Eleonora Di Valentino, Elia Battistelli, Emmanuel N. Saridakis, Eoin \\'O Colg\\'ain, Erminia Calabrese, Fabio Finelli, Florian Niedermann, Fran\\c{c}ois R. Bouchet, Francesco Pace, Francesco Piacentini, Francis-Yan Cyr-Racine, Hendrik Hildebrandt, Ian Harrison, Jacques Delabrouille, Javier de Cruz P\\'erez, Jens Chluba, Jessica Muir, Jian-Min Wang, Joan Sol\\`a, Jo Dunkley, Joseph Silk, Julien Lesgourgues, Laura Mersini-Houghton, Licia Verde, Lloyd Knox, Luca Amendola, Luca Lamagna, Luca Visinelli, Luis A. Anchordoqui, Luke Hart, Marc Kamionkowski, Marco Bruni, Marco Raveri, Marika Asgari, Mario Ballardini, Martin S. Sloth, Matteo Lucca, Micol Benetti, Mikhail M. Ivanov, Nikki Arendse, Noemi Frusciante, Olga Mena, Ozgur Akarsu, Paolo De Bernardis, Rafael C. Nunes, Sabino Matarrese, Salvatore Capozziello, Shahab Joudaki, Silvia Masi, Simon Birrer, Spyros Basilakos, Supriya Pan, Suresh Kumar, Tanvi Karwal, Tristan L. Smith, Valeria Pettorino, Valerio Marra, Vincenzo Salzano, Vivian Miranda, Vivian Poulin, Weiqiang Yang, Wendy Freedman, Will Handley, Yacine Ali-Haimoud","submitted_at":"2020-08-25T21:41:42Z","abstract_excerpt":"The standard $\\Lambda$ Cold Dark Matter cosmological model provides a wonderful fit to current cosmological data, but a few tensions and anomalies became statistically significant with the latest data analyses. While these anomalies could be due to the presence of systematic errors in the experiments, they could also indicate the need for new physics beyond the standard model. In this Letter of Interest we focus on the tension of the Planck data with weak lensing measurements and redshift surveys, about the value of the matter energy density $\\Omega_m$, and the amplitude or rate of the growth "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2008.11285","kind":"arxiv","version":4},"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/2008.11285/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"}