{"paper":{"title":"Exclusion of Leptophilic Dark Matter Models using XENON100 Electronic Recoil Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"astro-ph.CO","authors_text":"A. Behrens, A. Brown, A. D. Ferella, A. Di Giovanni, A. Fieguth, A. J. Melgarejo Fernandez, A. Kish, A. Lyashenko, A. Molinario, A. P. Colijn, A. Rizzo, A. Teymourian, A. Tiseni, B. Bauermeister, B. Kaminsky, B. Miguez, C. Balan, C. Geis, C. Grignon, C. Levy, C. Reuter, C. Tunnell, C. Weinheimer, D. Coderre, D. Lellouch, D. Mayani Paras, D. Thers, E. Brown, E. Duchovni, E. Gross, E. Pantic, F. Agostini, F. Arneodo, F. Gao, F. Kaether, F. Piastra, F. V. Massoli, G. Bruno, G. Kessler, G. Morana, G. Plante, G. Sartorelli, G. Trinchero, H. Contreras, H. Landsman, H. Simgen, H. Wang, J. A. M. Lopes, J. Masbou, J. M. F. dos Santos, J. M. R. Cardoso, J. Naganoma, J. P. Cussonneau, J. Pienaar, J. Schreiner, K. Arisaka, K. Ni, L. Arazi, L. Baudis, L. Buetikofer, L. Levinson, L. Rauch, L. Scotto Lavina, L. W. Goetzke, M. Alfonsi, M. Auger, M. Cervantes, M. Garbini, M. Le Calloch, M. Lindner, M. Messina, M. Murra, M. P. Decowski, M. Schumann, M. Selvi, M. Weber, N. Priel, O. Vitells, P. Barrow, 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, The XENON Collaboration: E. Aprile, T. Marrodan Undagoitia, U. Oberlack, W. Fulgione, W. Hampel, Y. Meng","submitted_at":"2015-07-28T12:56:07Z","abstract_excerpt":"Laboratory experiments searching for galactic dark matter particles scattering off nuclei have so far not been able to establish a discovery. We use data from the XENON100 experiment to search for dark matter interacting with electrons. With no evidence for a signal above the low background of our experiment, we exclude a variety of representative dark matter models that would induce electronic recoils. For axial-vector couplings to electrons, we exclude cross-sections above 6x10^(-35) cm^2 for particle masses of m_chi = 2 GeV/c^2. Independent of the dark matter halo, we exclude leptophilic mo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.07747","kind":"arxiv","version":1},"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"}