{"paper":{"title":"Physics reach of the XENON1T dark matter experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"physics.ins-det","authors_text":"A. Breskin, A. Brown, A. D. Ferella, A. Di Giovanni, A. Fieguth, A. J. Melgarejo Fernandez, A. Kish, A. Lyashenko, A. Manfredini, A. Molinario, A. P. Colijn, A. Rizzo, A. Stein, A. Tiseni, B. Bauermeister, B. Kaminsky, B. Miguez, B. Pelssers, C. Balan, C. Geis, C. Grignon, C. Hasterok, C. Levy, C. Reuter, C. Tunnell, C. Weinheimer, D. Cichon, D. Coderre, D. Franco, D. Lellouch, D. Mayani, D. Thers, E. Brown, E. Duchovni, E. Gross, F. Agostini, F. Arneodo, F. D. Amaro, F. Kaether, F. Piastra, F. V. Massoli, G. Bruno, G. Kessler, G. Plante, G. Sartorelli, G. Trinchero, H. Contreras, H. Landsman, H. Simgen, H. Wang, J. Aalbers, J. A. M. Lopes, J. Conrad, J. Masbou, J. M. F. dos Santos, J. M. R. Cardoso, J. Naganoma, J. P. Cussonneau, J. Pienaar, J. Schreiner, J. Wulf, K. Micheneau, L. Arazi, L. Baudis, L. B\\\"utikofer, L. Levinson, L. Rauch, L. Scotto Lavina, L. W. Goetzke, M. Alfonsi, M. Anthony, M. Cervantes, M. Galloway, M. Garbini, M. Le Calloch, M. Lindner, M. Messina, M. Murra, M. P. Decowski, M. Scheibelhut, M. Schumann, M. Selvi, M. von Sivers, M. Weber, N. Priel, N. Rupp, P. Barrow, P. Breur, P. de Perio, P. Di Gangi, P. Pakarha, P. Shagin, R. Budnik, R. F. Lang, R. Itay, R. Persiani, R. Wall, S. Bruenner, S. E. A. Orrigo, S. Fattori, S. Lindemann, S. MacMullin, S. Reichard, S. Rosendahl, S. Schindler, T. Berger, The XENON Collaboration: E. Aprile, T. Marrod\\'an Undagoitia, U. Oberlack, W. Fulgione, W. Hampel, Y. Meng, Y. Wei, Y. Zhang, Z. Greene","submitted_at":"2015-12-23T14:52:50Z","abstract_excerpt":"The XENON1T experiment is currently in the commissioning phase at the Laboratori Nazionali del Gran Sasso, Italy. In this article we study the experiment's expected sensitivity to the spin-independent WIMP-nucleon interaction cross section, based on Monte Carlo predictions of the electronic and nuclear recoil backgrounds.\n  The total electronic recoil background in $1$ tonne fiducial volume and ($1$, $12$) keV electronic recoil equivalent energy region, before applying any selection to discriminate between electronic and nuclear recoils, is $(1.80 \\pm 0.15) \\cdot 10^{-4}$ ($\\rm{kg} \\cdot day \\"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.07501","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":""},"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"}