Dark Matter Results from 225 Live Days of XENON100 Data

E. Aprile(Columbia University), M. Alfonsi(National Institute for Subatomic Physics), K. Arisaka(University of California, Los Angeles), F. Arneodo(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso), Cătălin Balan(University of Coimbra), L. Baudis(University of Zurich), B. Bauermeister(Johannes Gutenberg University Mainz), A. Behrens(University of Zurich), P. Beltrame(University of California, Los Angeles), K. Bokeloh(University of Münster), A. Brown(University of Münster), G. Bruno(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso), R. Budnik(Columbia University), J. M. R. Cardoso(University of Coimbra), W.-T. Chen(Centre National de la Recherche Scientifique), Bernard C. K. Choi(Columbia University), D. Cline(University of California, Los Angeles), A. P. Colijn(National Institute for Subatomic Physics), Hugo Contreras(Columbia University), J. P. Cussonneau(Centre National de la Recherche Scientifique), M. P. Decowski(National Institute for Subatomic Physics), E. Duchovni(Weizmann Institute of Science), S. Fattori(Johannes Gutenberg University Mainz), A. D. Ferella(University of Zurich), W. Fulgione(Osservatorio Astrofisico di Torino), F. Gao(Shanghai Jiao Tong University), M. Garbini(Istituto Nazionale di Fisica Nucleare, Sezione di Bologna), C. Ghag(University of California, Los Angeles), Karl Giboni(Columbia University), L. W. Goetzke(Columbia University), C. Grignon(Johannes Gutenberg University Mainz), E. Gross(Weizmann Institute of Science), W. Hampel(Max Planck Institute for Nuclear Physics), F. Kaether(Max Planck Institute for Nuclear Physics), A. Kish(University of Zurich), J. Lamblin(Centre National de la Recherche Scientifique), H. Landsman(Weizmann Institute of Science), R. F. Lang(Purdue University West Lafayette), M. Le Calloch(Centre National de la Recherche Scientifique), C. Levy(University of Münster), K. E. Lim(Columbia University), Q. Lin(Shanghai Jiao Tong University), S. Lindemann(Max Planck Institute for Nuclear Physics), M. Lindner(Max Planck Institute for Nuclear Physics), J. A. M. Lopes(University of Coimbra), K. Lung(University of California, Los Angeles), T. Marrodán Undagoitia(University of Zurich), Fabio Valerio Massoli(Istituto Nazionale di Fisica Nucleare, Sezione di Bologna), A. J. Melgarejo Fernandez(Columbia University), Yue Meng(University of California, Los Angeles), A. Molinario(Osservatorio Astrofisico di Torino), E. Nativ(Weizmann Institute of Science), K. Ni(Shanghai Jiao Tong University), U. Oberlack(Johannes Gutenberg University Mainz), S. E. A. Orrigo(University of Coimbra), E. Pantic(University of California, Los Angeles), R. Persiani(Istituto Nazionale di Fisica Nucleare, Sezione di Bologna), G. Plante(Columbia University), N. Priel(Weizmann Institute of Science), A. Rizzo(Columbia University), S. S. E. Rosendahl(University of Münster), J.M.F. dos Santos(University of Coimbra), G. Sartorelli(Istituto Nazionale di Fisica Nucleare, Sezione di Bologna), J. Schreiner(Max Planck Institute for Nuclear Physics), M. Schümann(University of Zurich), L. Scotto Lavina(Centre National de la Recherche Scientifique), P. R. Scovell(University of California, Los Angeles), M. Selvi(Istituto Nazionale di Fisica Nucleare, Sezione di Bologna), P. Shagin(Rice University), H. Simgen(Max Planck Institute for Nuclear Physics), A. Teymourian(University of California, Los Angeles), D. Thers(Centre National de la Recherche Scientifique), O. Vitells(Weizmann Institute of Science), H. Wang(University of California, Los Angeles), M. Weber(Max Planck Institute for Nuclear Physics), C. Weinheimer(University of Münster)
Physical Review Letters
November 2, 2012
Cited by 1,415Open Access
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Abstract

We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso for 13 months during 2011 and 2012. XENON100 features an ultralow electromagnetic background of $(5.3\ifmmode\pm\else\textpm\fi{}0.6)\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}3}\text{ }\text{ }\mathrm{events}/({\mathrm{keV}}_{\mathrm{ee}}\ifmmode\times\else\texttimes\fi{}\mathrm{kg}\ifmmode\times\else\texttimes\fi{}\mathrm{day})$ in the energy region of interest. A blind analysis of $224.6\text{ }\mathrm{\text{live days}}\ifmmode\times\else\texttimes\fi{}34\text{ }\text{ }\mathrm{kg}$ exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the predefined nuclear recoil energy range of $6.6--30.5\text{ }\text{ }{\mathrm{keV}}_{\mathrm{nr}}$ are consistent with the background expectation of ($1.0\ifmmode\pm\else\textpm\fi{}0.2$) events. A profile likelihood analysis using a $6.6--43.3\text{ }\text{ }{\mathrm{keV}}_{\mathrm{nr}}$ energy range sets the most stringent limit on the spin-independent elastic weakly interacting massive particle--nucleon scattering cross section for weakly interacting massive particle masses above $8\text{ }\text{ }\mathrm{GeV}/{c}^{2}$, with a minimum of $2\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}45}\text{ }\text{ }{\mathrm{cm}}^{2}$ at $55\text{ }\text{ }\mathrm{GeV}/{c}^{2}$ and 90% confidence level.


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