中文
相关论文

相关论文: Muon-induced neutrons do not explain the DAMA data

200 篇论文

We present the first search for dark matter-induced delayed coincidence signals in a dual-phase xenon time projection chamber, using the 224.6 live days of the XENON100 science run II. This very distinct signature is predicted in the…

宇宙学与河外天体物理 · 物理学 2017-11-01 XENON collaboration , E. Aprile , J. Aalbers , F. Agostini , M. Alfonsi , F. D. Amaro , M. Anthony , F. Arneodo , P. Barrow , L. Baudis , B. Bauermeister , M. L. Benabderrahmane , T. Berger , P. A. Breur , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , L. Bütikofer , J. Calvén , J. M. R. Cardoso , M. Cervantes , D. Cichon , D. Coderre , A. P. Colijn , J. Conrad , J. P. Cussonneau , M. P. Decowski , P. de Perio , P. Di Gangi , A. Di Giovanni , S. Diglio , G. Eurin , J. Fei , A. D. Ferella , A. Fieguth , D. Franco , W. Fulgione , A. Gallo Rosso , M. Galloway , F. Gao , M. Garbini , C. Geis , L. W. Goetzke , Z. Greene , C. Grignon , C. Hasterok , E. Hogenbirk , R. Itay , B. Kaminsky , G. Kessler , A. Kish , H. Landsman , R. F. Lang , D. Lellouch , L. Levinson , Q. Lin , S. Lindemann , M. Lindner , F. Lombardi , J. A. M. Lopes , A. Manfredini , I. Maris , T. Marrodán Undagoitia , J. Masbou , F. V. Massoli , D. Masson , D. Mayani , M. Messina , K. Micheneau , A. Molinario , M. Murra , J. Naganoma , K. Ni , U. Oberlack , P. Pakarha , B. Pelssers , R. Persiani , F. Piastra , J. Pienaar , V. Pizzella , M. -C. Piro , G. Plante , N. Priel , L. Rauch , S. Reichard , C. Reuter , A. Rizzo , S. Rosendahl , N. Rupp , J. M. F. dos Santos , G. Sartorelli , M. Scheibelhut , S. Schindler , J. Schreiner , M. Schumann , L. Scotto Lavina , M. Selvi , P. Shagin , M. Silva , H. Simgen , M. v. Sivers , A. Stein , D. Thers , A. Tiseni , G. Trinchero , C. Tunnell , M. Vargas , H. Wang , Y. Wei , C. Weinheimer , J. Wulf , J. Ye , Y. Zhanga

Inelastic dark matter, in which WIMP-nucleus scatterings occur through a transition to an excited WIMP state ~ 100 keV above the ground state, provides a compelling explanation of the DAMA annual modulation signal. We demonstrate that the…

高能物理 - 唯象学 · 物理学 2009-05-22 Spencer Chang , Graham D. Kribs , David Tucker-Smith , Neal Weiner

The flux of neutrino-induced muons has been measured with the MACRO detector. Different event topologies have been detected, due to neutrino interactions in the apparatus and in the rock below it. The upward-throughgoing muon sample is the…

高能物理 - 实验 · 物理学 2007-05-23 Paolo Bernardini

The simplest version of the daemon paradigm suggests the modulated 2-6-keV range events in DAMA/NaI and DAMA/LIBRA detectors are caused by the iodine ions knocked out elastically by the electrically neutral c-daemons moving with V = 30-50…

天体物理学 · 物理学 2009-11-13 E. M. Drobyshevski

The neutron background at the underground laboratory at Boulby - a site for several dark matter experiments - is discussed. Special emphasis is put on the neutron background produced by cosmic-ray muons. The most recent versions of the muon…

A measurement of the flux of neutrino-induced muons using the MACRO detector is presented. Different event topologies, corresponding to different neutrino parent energies can be detected. The upward throughgoing muon sample is the larger…

高能物理 - 实验 · 物理学 2008-11-26 F. Ronga

The XENON100 experiment has recently completed a dark matter run with 100.9 live-days of data, taken from January to June 2010. Events in a 48kg fiducial volume in the energy range between 8.4 and 44.6 keVnr have been analyzed. A total of…

Muon-induced neutrons can lead to potentially irreducible backgrounds in rare event search experiments. We have investigated the implication of laboratory depth on the muon induced background in a future dark matter experiment capable of…

高能物理 - 实验 · 物理学 2022-11-15 Viktor Pěč , Vitaly A. Kudryavtsev

Presented here are results of simulations of neutron background performed for a time projection chamber acting as a particle dark matter detector in an underground laboratory. The investigated background includes neutrons from rock and…

Cosmic muon induced neutrons are a major source of background for low countrate experiments like neutrino oscillation or dark matter searches. Especially at shallow sites these neutrons are the limiting factor for the ultimate sensitivity…

高能物理 - 实验 · 物理学 2017-08-23 J. Wolf

Ambient radiation background contributed by the penetrating cosmic ray particles and the radionuclides present in the rock materials have been measured at an underground laboratory located inside a mine at 555 m depth. The laboratory is…

天体物理仪器与方法 · 物理学 2022-03-14 Sayan Ghosh , Shubham Dutta , Naba Kumar Mondal , Satyajit Saha

The KArlsruhe TRItium Neutrino (KATRIN) experiment aims to make a model-independent determination of the effective electron antineutrino mass with a sensitivity of 0.2 eV/c$^{2}$. It investigates the kinematics of $\beta$-particles from…

仪器与探测器 · 物理学 2019-01-11 K. Altenmüller , M. Arenz , W. -J. Baek , M. Beck , A. Beglarian , J. Behrens , T. Bergmann , A. Berlev , U. Besserer , K. Blaum , S. Bobien , T. Bode , B. Bornschein , L. Bornschein , T. Brunst , N. Buzinsky , S. Chilingaryan , W. Q. Choi , M. Deffert , P. J. Doe , O. Dragoun , G. Drexlin , S. Dyba , F. Edzards , K. Eitel , E. Ellinger , R. Engel , S. Enomoto , M. Erhard , D. Eversheim , M. Fedkevych , J. A. Formaggio , F. M. Fränkle , G. B. Franklin , F. Friedel , A. Fulst , W. Gil , F. Glück , A. Gonzalez Ureña , S. Grohmann , R. Grössle , R. Gumbsheimer , M. Hackenjos , V. Hannen , F. Harms , N. Haußmann , F. Heizmann , K. Helbing , W. Herz , S. Hickford , D. Hilk , D. Hillesheimer , M. A. Howe , A. Huber , A. Jansen , J. Kellerer , N. Kernert , L. Kippenbrock , M. Kleesiek , M. Klein , A. Kopmann , M. Korzeczek , A. Kovalík , B. Krasch , M. Kraus , L. Kuckert , T. Lasserre , O. Lebeda , B. Leiber , J. Letnev , J. Linek , A. Lokhov , M. Machatschek , A. Marsteller , E. L. Martin , S. Mertens , S. Mirz , B. Monreal , H. Neumann , S. Niemes , A. Off , A. Osipowicz , E. Otten , D. S. Parno , A. Pollithy , A. W. P. Poon , F. Priester , P. C. -O. Ranitzsch , O. Rest , R. Rink , R. G. H. Robertson , F. Roccati , C. Rodenbeck , M. Röllig , C. Röttele , P. Rovedo , M. Ryšavý , R. Sack , A. Saenz , L. Schimpf , K. Schlösser , M. Schlösser , K. Schönung , M. Schrank , H. Seitz-Moskaliuk , J. Sentkerestiová , V. Sibille , M. Slezák , M. Steidl , N. Steinbrink , M. Sturm , M. Suchopar , M. Suesser , H. H. Telle , L. A. Thorne , T. Thümmler , N. Titov , I. Tkachev , N. Trost , K. Valerius , D. Vénos , R. Vianden , A. P. Vizcaya Hernández , N. Wandkowsky , M. Weber , C. Weinheimer , C. Weiss , S. Welte , J. Wendel , J. F. Wilkerson , J. Wolf , S. Wüstling , S. Zadoroghny , G. Zeller

We report on a search for electromagnetic and/or hadronic showers (cascades) induced by a diffuse flux of neutrinos with energies between 5 TeV and 300 TeV from extraterrestrial sources. Cascades may be produced by matter interactions of…

天体物理学 · 物理学 2011-08-31 J. Ahrens

The DAMA experiment clearly observes a small oscillatory signal. The observed yearly modulation is in phase with the Earth's motion around the Sun. Recent reference [Vavra, 2014] suggested that the DAMA experiment observes a WIMP of much…

天体物理仪器与方法 · 物理学 2014-01-28 J. Va'vra

The CoGeNT collaboration has reported evidence of an annual modulation in its first fifteen months of data. Here we compare the amplitude and phase of this signal to the modulation observed by the DAMA collaboration, assuming that both…

高能物理 - 唯象学 · 物理学 2011-09-14 Christopher McCabe

Experimental observations and theoretical arguments point out that Dark Matter (DM) particles are one of the most prominent component of the Universe. This motivated the pioneer DAMA experiment to investigate the presence of these particles…

The flux of muons induced by atmospheric neutrinos has been measured with the MACRO detector. Different event topologies have been detected, due to neutrino interactions in the apparatus and in the rock below it. The upward-throughgoing…

高能物理 - 实验 · 物理学 2007-05-23 Paolo Bernardini

Renewed international interest in muon colliders motivates the continued investigation of the impacts of beam-induced background on detector performance. This continues the effort initiated by the Muon Accelerator Program and carried out…

Simulations of the neutron background for future large-scale particle dark matter detectors are presented. Neutrons were generated in rock and detector elements via spontaneous fission and (alpha,n) reactions, and by cosmic-ray muons. The…

We present a comprehensive Monte Carlo simulation of muon-induced backgrounds for the Colorado Underground Research Institute (CURIE), a shallow-underground facility with $\approx 415$~m.w.e. overburden. Using coupled \textsc{mute} and…