English
Related papers

Related papers: Finding Dark Matter Faster with Explicit Profile L…

200 papers

We report the first dark matter search results from XENON1T, a $\sim$2000-kg-target-mass dual-phase (liquid-gas) xenon time projection chamber in operation at the Laboratori Nazionali del Gran Sasso in Italy and the first ton-scale detector…

Cosmology and Nongalactic Astrophysics · Physics 2017-11-27 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 , 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 , W. Fulgione , A. Gallo Rosso , M. Galloway , F. Gao , M. Garbini , R. Gardner , C. Geis , L. W. Goetzke , L. Grandi , Z. Greene , C. Grignon , C. Hasterok , E. Hogenbirk , J. Howlett , R. Itay , B. Kaminsky , S. Kazama , 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. Mariş , T. Marrodán Undagoitia , J. Masbou , F. V. Massoli , D. Masson , D. Mayani , M. Messina , K. Micheneau , A. Molinario , K. Morå , 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 , B. Riedel , A. Rizzo , S. Rosendahl , N. Rupp , R. Saldanha , J. M. F. dos Santos , G. Sartorelli , M. Scheibelhut , S. Schindler , J. Schreiner , M. Schumann , L. Scotto Lavina , M. Selvi , P. Shagin , E. Shockley , M. Silva , H. Simgen , M. v. Sivers , A. Stein , S. Thapa , D. Thers , A. Tiseni , G. Trinchero , C. Tunnell , M. Vargas , N. Upole , H. Wang , Z. Wang , Y. Wei , C. Weinheimer , J. Wulf , J. Ye , Y. Zhang , T. Zhu

Experimental efforts searching for dark matter particles over the last few decades have ruled out many candidates led by the new generation of tonne-scale liquid xenon. For light dark matter, hydrogen could be a better target than xenon as…

The Large Underground Xenon (LUX) dark matter search experiment is currently being deployed at the Homestake Laboratory in South Dakota. We will highlight the main elements of design which make the experiment a very strong competitor in the…

The XENON100 experiment, in operation at the Laboratori Nazionali del Gran Sasso in Italy, is designed to search for dark matter WIMPs scattering off 62 kg of liquid xenon in an ultra-low background dual-phase time projection chamber. In…

The energy and electric field dependence of pulse shape discrimination in liquid xenon have been measured in a 10 gm two-phase xenon time projection chamber. We have demonstrated the use of the pulse shape and charge-to-light ratio…

Instrumentation and Methods for Astrophysics · Physics 2015-05-13 J. Kwong , P. Brusov , T. Shutt , C. E. Dahl , A. I. Bolozdynya , A. Bradley

Motivated by the current interest in employing quantum sensors on Earth and in space to conduct searches for new physics, we provide a perspective on the suitability of large-mass levitated optomechanical systems for observing dark matter…

We show how the material used in direct detection experiments of Dark Matter (DM), in the presence of a signal of it, can afford one with the possibility of extracting the nature of the underlying candidate. We do so for the case of a…

High Energy Physics - Phenomenology · Physics 2021-05-19 Yaşar Hiçyılmaz , Stefano Moretti

Cosmological mechanisms that yield ultralight dark matter are insensitive to the intrinsic parity of a bosonic dark matter candidate, but that same quantity plays a crucial role in a direct detection experiment. The modification of…

High Energy Physics - Phenomenology · Physics 2021-09-20 Christopher M. Donohue , Susan Gardner , Wolfgang Korsch

Dark matter (DM) is currently searched for with a variety of detection strategies. Accelerator searches are particularly promising, but even if Weakly Interacting Massive Particles (WIMPs) are found at the Large Hadron Collider (LHC), it…

High Energy Physics - Phenomenology · Physics 2010-10-13 Gianfranco Bertone , David G. Cerdeno , Mattia Fornasa , Roberto Ruiz de Austri , Roberto Trotta

Direct detection experiments for light dark matter are making enormous leaps in reaching previously unexplored model space. Several recent proposals rely on collective excitations, where the experimental sensitivity is highly dependent on…

High Energy Physics - Phenomenology · Physics 2021-10-22 Sinead M. Griffin , Katherine Inzani , Tanner Trickle , Zhengkang Zhang , Kathryn M. Zurek

We describe the design and assembly of the LUX-ZEPLIN experiment, a direct detection search for cosmic WIMP dark matter particles. The centerpiece of the experiment is a large liquid xenon time projection chamber sensitive to low energy…

Instrumentation and Detectors · Physics 2019-11-05 The LZ Collaboration , D. S. Akerib , C. W. Akerlof , D. Yu. Akimov , A. Alquahtani , S. K. Alsum , T. J. Anderson , N. Angelides , H. M. Araújo , A. Arbuckle , J. E. Armstrong , M. Arthurs , H. Auyeung , X. Bai , A. J. Bailey , J. Balajthy , S. Balashov , J. Bang , M. J. Barry , J. Barthel , D. Bauer , P. Bauer , A. Baxter , J. Belle , P. Beltrame , J. Bensinger , T. Benson , E. P. Bernard , A. Bernstein , A. Bhatti , A. Biekert , T. P. Biesiadzinski , B. Birrittella , K. E. Boast , A. I. Bolozdynya , E. M. Boulton , B. Boxer , R. Bramante , S. Branson , P. Brás , M. Breidenbach , J. H. Buckley , V. V. Bugaev , R. Bunker , S. Burdin , J. K. Busenitz , J. S. Campbell , C. Carels , D. L. Carlsmith , B. Carlson , M. C. Carmona-Benitez , M. Cascella , C. Chan , J. J. Cherwinka , A. A. Chiller , C. Chiller , N. I. Chott , A. Cole , J. Coleman , D. Colling , R. A. Conley , A. Cottle , R. Coughlen , W. W. Craddock , D. Curran , A. Currie , J. E. Cutter , J. P. da Cunha , C. E. Dahl , S. Dardin , S. Dasu , J. Davis , T. J. R. Davison , L. de Viveiros , N. Decheine , A. Dobi , J. E. Y. Dobson , E. Druszkiewicz , A. Dushkin , T. K. Edberg , W. R. Edwards , B. N. Edwards , J. Edwards , M. M. Elnimr , W. T. Emmet , S. R. Eriksen , C. H. Faham , A. Fan , S. Fayer , S. Fiorucci , H. Flaecher , I. M. Fogarty Florang , P. Ford , V. B. Francis , F. Froborg , T. Fruth , R. J. Gaitskell , N. J. Gantos , D. Garcia , A. Geffre , V. M. Gehman , R. Gelfand , J. Genovesi , R. M. Gerhard , C. Ghag , E. Gibson , M. G. D. Gilchriese , S. Gokhale , B. Gomber , T. G. Gonda , A. Greenall , S. Greenwood , G. Gregerson , M. G. D. van der Grinten , C. B. Gwilliam , C. R. Hall , D. Hamilton , S. Hans , K. Hanzel , T. Harrington , A. Harrison , C. Hasselkus , S. J. Haselschwardt , D. Hemer , S. A. Hertel , J. Heise , S. Hillbrand , O. Hitchcock , C. Hjemfelt , M. D. Hoff , B. Holbrook , E. Holtom , J. Y-K. Hor , M. Horn , D. Q. Huang , T. W. Hurteau , C. M. Ignarra , M. N. Irving , R. G. Jacobsen , O. Jahangir , S. N. Jeffery , W. Ji , M. Johnson , J. Johnson , P. Johnson , W. G. Jones , A. C. Kaboth , A. Kamaha , K. Kamdin , V. Kasey , K. Kazkaz , J. Keefner , D. Khaitan , M. Khaleeq , A. Khazov , A. V. Khromov , I. Khurana , Y. D. Kim , W. T. Kim , C. D. Kocher , A. M. Konovalov , L. Korley , E. V. Korolkova , M. Koyuncu , J. Kras , H. Kraus , S. W. Kravitz , H. J. Krebs , L. Kreczko , B. Krikler , V. A. Kudryavtsev , A. V. Kumpan , S. Kyre , A. R. Lambert , B. Landerud , N. A. Larsen , A. Laundrie , E. A. Leason , H. S. Lee , J. Lee , C. Lee , B. G. Lenardo , D. S. Leonard , R. Leonard , K. T. Lesko , C. Levy , J. Li , Y. Liu , J. Liao , F. -T. Liao , J. Lin , A. Lindote , R. Linehan , W. H. Lippincott , R. Liu , X. Liu , C. Loniewski , M. I. Lopes , B. López Paredes , W. Lorenzon , D. Lucero , S. Luitz , J. M. Lyle , C. Lynch , P. A. Majewski , J. Makkinje , D. C. Malling , A. Manalaysay , L. Manenti , R. L. Mannino , N. Marangou , D. J. Markley , P. MarrLaundrie , T. J. Martin , M. F. Marzioni , C. Maupin , C. T. McConnell , D. N. McKinsey , J. McLaughlin , D. -M. Mei , Y. Meng , E. H. Miller , Z. J. Minaker , E. Mizrachi , J. Mock , D. Molash , A. Monte , M. E. Monzani , J. A. Morad , E. Morrison , B. J. Mount , A. St. J. Murphy , D. Naim , A. Naylor , C. Nedlik , C. Nehrkorn , H. N. Nelson , J. Nesbit , F. Neves , J. A. Nikkel , J. A. Nikoleyczik , A. Nilima , J. O'Dell , H. Oh , F. G. O'Neill , K. O'Sullivan , I. Olcina , M. A. Olevitch , K. C. Oliver-Mallory , L. Oxborough , A. Pagac , D. Pagenkopf , S. Pal , K. J. Palladino , V. M. Palmaccio , J. Palmer , M. Pangilinan , S. J. Patton , E. K. Pease , B. P. Penning , G. Pereira , C. Pereira , I. B. Peterson , A. Piepke , S. Pierson , S. Powell , R. M. Preece , K. Pushkin , Y. Qie , M. Racine , B. N. Ratcliff , J. Reichenbacher , L. Reichhart , C. A. Rhyne , A. Richards , Q. Riffard , G. R. C. Rischbieter , J. P. Rodrigues , H. J. Rose , R. Rosero , P. Rossiter , R. Rucinski , G. Rutherford , D. Rynders , J. S. Saba , L. Sabarots , D. Santone , M. Sarychev , A. B. M. R. Sazzad , R. W. Schnee , M. Schubnell , P. R. Scovell , M. Severson , D. Seymour , S. Shaw , G. W. Shutt , T. A. Shutt , J. J. Silk , C. Silva , K. Skarpaas , W. Skulski , A. R. Smith , R. J. Smith , R. E. Smith , J. So , M. Solmaz , V. N. Solovov , P. Sorensen , V. V. Sosnovtsev , I. Stancu , M. R. Stark , S. Stephenson , N. Stern , A. Stevens , T. M. Stiegler , K. Stifter , R. Studley , T. J. Sumner , K. Sundarnath , P. Sutcliffe , N. Swanson , M. Szydagis , M. Tan , W. C. Taylor , R. Taylor , D. J. Taylor , D. Temples , B. P. Tennyson , P. A. Terman , K. J. Thomas , J. A. Thomson , D. R. Tiedt , M. Timalsina , W. H. To , A. Tomás , T. E. Tope , M. Tripathi , D. R. Tronstad , C. E. Tull , W. Turner , L. Tvrznikova , M. Utes , U. Utku , S. Uvarov , J. Va'vra , A. Vacheret , A. Vaitkus , J. R. Verbus , T. Vietanen , E. Voirin , C. O. Vuosalo , S. Walcott , W. L. Waldron , K. Walker , J. J. Wang , R. Wang , L. Wang , Y. Wang , J. R. Watson , J. Migneault , S. Weatherly , R. C. Webb , W. -Z. Wei , M. While , R. G. White , J. T. White , D. T. White , T. J. Whitis , W. J. Wisniewski , K. Wilson , M. S. Witherell , F. L. H. Wolfs , J. D. Wolfs , D. Woodward , S. D. Worm , X. Xiang , Q. Xiao , J. Xu , M. Yeh , J. Yin , I. Young , C. Zhang

Forecasting the signal discrimination power of dark matter (DM) searches is commonly limited to a set of arbitrary benchmark points. We introduce new methods for benchmark-free forecasting that instead allow an exhaustive exploration and…

High Energy Physics - Phenomenology · Physics 2018-11-14 Thomas D. P. Edwards , Bradley J. Kavanagh , Christoph Weniger

Direct and indirect dark matter detection relies on the scattering of the dark matter candidate on nucleons or nuclei. Here, attention is focused on dark matter candidates (neutralinos) predicted in the minimal supersymmetric standard model…

High Energy Physics - Phenomenology · Physics 2014-11-17 John Ellis , Andrew Ferstl , Keith A. Olive

We demonstrate that current and planned underground neutrino experiments could offer a powerful probe of few-MeV dark matter when combined with a nearby high-intensity low-to-medium energy electron accelerator. This experimental setup, an…

High Energy Physics - Phenomenology · Physics 2015-11-18 Eder Izaguirre , Gordan Krnjaic , Maxim Pospelov

We compute the neutralino direct detection rate in non-standard cosmological scenarios where neutralinos account for the dark matter of the Universe. Significant differences are found when such rates are compared with those predicted by the…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Gelmini , P. Gondolo , A. Soldatenko , C. E. Yaguna

Dark matter detectors using the liquid noble gases xenon and argon as WIMP targets have evolved rapidly in the last decade and will continue to play a major role in the field. Due to the possibility to scale these detectors to larger masses…

Instrumentation and Methods for Astrophysics · Physics 2012-06-12 Marc Schumann

The known direction of motion of dark matter particles relative to the Earth may be a key for their unambiguous identification even in the presence of backgrounds. We describe a prototype detector that is able to reconstruct direction…

The XENON10 experiment at the Gran Sasso National Laboratory uses a 15 kg xenon dual phase time projection chamber (XeTPC) to search for dark matter weakly interacting massive particles (WIMPs). The detector measures simultaneously the…

Gas-filled Time Projection Chambers (TPCs) with Gas Electron Multipliers (GEMs) and pixels appear suitable for direction-sensitive WIMP dark matter searches. We present the background and motivation for our work on this technology, past and…

Instrumentation and Methods for Astrophysics · Physics 2015-05-30 S. E. Vahsen , H. Feng , M. Garcia-Sciveres , I. Jaegle , J. Kadyk , Y. Nguyen , M. Rosen , S. Ross , T. Thorpe , J. Yamaoka