Related papers: The XENON1T Dark Matter Search Experiment

Light WIMP search in XMASS

A search for light dark matter using low-threshold data from the single phase liquid xenon scintillation detector XMASS, has been conducted. Using the entire 835 kg inner volume as target, the analysis threshold can be lowered to 0.3 keVee…

Cosmology and Nongalactic Astrophysics · Physics 2013-01-31 K. Abe , K. Hieda , K. Hiraide , S. Hirano , Y. Kishimoto , K. Kobayashi , S. Moriyama , K. Nakagawa , M. Nakahata , H. Ogawa , N. Oka , H. Sekiya , A. Shinozaki Y. Suzuki , A. Takeda , O. Takachio , K. Ueshima , D. Umemoto , M. Yamashita , B. S. Yang , S. Tasaka , J. Liu , K. Martens , K. Hosokawa , K. Miuchi , A. Murata , Y. Onishi , Y. Otsuka , Y. Takeuchi , Y. H. Kim , K. B. Lee , M. K. Lee , J. S. Lee , Y. Fukuda , Y. Itow , K. Masuda , Y. Nishitani , H. Takiya , H. Uchida , N. Y. Kim , Y. D. Kim , F. Kusaba , D. Motoki , K. Nishijima , K. Fujii , I. Murayama , S. Nakamura

XENON: a 1 tonne Liquid Xenon Experiment for a Sensitive Dark Matter Search

XENON is a novel liquid xenon experiment concept for a sensitive dark matter search using a 1-tonne active target, distributed in an array of ten independent time projection chambers. The design relies on the simultaneous detection of…

Astrophysics · Physics 2017-08-23 E. Aprile , E. A. Baltz , A. Curioni , K-L. Giboni , C. J. Hailey , L. Hui , M. Kobayashi , K. Ni , W. W. Craig , R. J. Gaitskell , U. Oberlack , T. Shutt

Optical response of highly reflective film used in the water Cherenkov muon veto of the XENON1T dark matter experiment

The XENON1T experiment is the most recent stage of the XENON Dark Matter Search, aiming for the direct detection of Weakly Interacting Massive Particles (WIMPs). To reach its projected sensitivity, the background has to be reduced by two…

Instrumentation and Detectors · Physics 2017-06-28 Christopher Geis , Cyril Grignon , Uwe Oberlack , Diego Ramírez García , Quirin Weitzel

Direct dark matter searches with the full data set of XMASS-I

Various WIMP dark matter searches using the full data set of XMASS-I, a single-phase liquid xenon detector, are reported in this paper. Stable XMASS-I data taking accumulated a total live time of 1590.9 days between November 20, 2013 and…

Cosmology and Nongalactic Astrophysics · Physics 2023-11-02 XMASS Collaboration , K. Abe , K. Hiraide , N. Kato , S. Moriyama , M. Nakahata , K. Sato , H. Sekiya , T. Suzuki , Y. Suzuki , A. Takeda , B. S. Yang , N. Y. Kim , Y. D. Kim , Y. H. Kim , Y. Itow , K. Martens , A. Mason , M. Yamashita , K. Miuchi , Y. Takeuchi , K. B. Lee , M. K. Lee , Y. Fukuda , H. Ogawa , K. Ichimura , Y. Kishimoto , K. Nishijima , K. Fushimi , B. D. Xu , K. Kobayashi , S. Nakamura

Physics reach of the XENON1T dark matter experiment

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,…

Instrumentation and Detectors · Physics 2016-04-25 The XENON collaboration , E. Aprile , J. Aalbers , F. Agostini , M. Alfonsi , F. D. Amaro , M. Anthony , L. Arazi , F. Arneodo , C. Balan , P. Barrow , L. Baudis , B. Bauermeister , T. Berger , P. Breur , A. Breskin , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , L. Bütikofer , J. M. R. Cardoso , M. Cervantes , D. Cichon , D. Coderre , A. P. Colijn , J. Conrad , H. Contreras , J. P. Cussonneau , M. P. Decowski , P. de Perio , P. Di Gangi , A. Di Giovanni , E. Duchovni , S. Fattori , A. D. Ferella , A. Fieguth , D. Franco , W. Fulgione , M. Galloway , M. Garbini , C. Geis , L. W. Goetzke , Z. Greene , C. Grignon , E. Gross , W. Hampel , C. Hasterok , R. Itay , F. Kaether , B. Kaminsky , G. Kessler , A. Kish , H. Landsman , R. F. Lang , D. Lellouch , L. Levinson , M. Le Calloch , C. Levy , S. Lindemann , M. Lindner , J. A. M. Lopes , A. Lyashenko , S. Macmullin , A. Manfredini , T. Marrodán Undagoitia , J. Masbou , F. V. Massoli , D. Mayani , A. J. Melgarejo Fernandez , Y. Meng , M. Messina , K. Micheneau , B. Miguez , A. Molinario , M. Murra , J. Naganoma , U. Oberlack , S. E. A. Orrigo , P. Pakarha , B. Pelssers , R. Persiani , F. Piastra , J. Pienaar , 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 , H. Simgen , A. Stein , D. Thers , A. Tiseni , G. Trinchero , C. Tunnell , M. von Sivers , R. Wall , H. Wang , M. Weber , Y. Wei , C. Weinheimer , J. Wulf , Y. Zhang

Dark Matter Results from 225 Live Days of XENON100 Data

We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso (LNGS) for 13 months during 2011 and 2012. XENON100 features an ultra-low electromagnetic background of (5.3…

Cosmology and Nongalactic Astrophysics · Physics 2013-03-21 XENON100 Collaboration , E. Aprile , M. Alfonsi , K. Arisaka , F. Arneodo , C. Balan , L. Baudis , B. Bauermeister , A. Behrens , P. Beltrame , K. Bokeloh , E. Brown , G. Bruno , R. Budnik , J. M. R. Cardoso , W. -T. Chen , B. Choi , D. Cline , A. P. Colijn , H. Contreras , J. P. Cussonneau , M. P. Decowski , E. Duchovni , S. Fattori , A. D. Ferella , W. Fulgione , F. Gao , M. Garbini , C. Ghag , K. -L. Giboni , L. W. Goetzke , C. Grignon , E. Gross , W. Hampel , F. Kaether , H. Kettling , A. Kish , J. Lamblin , H. Landsman , R. F. Lang , M. Le Calloch , C. Levy , K. E. Lim , Q. Lin , S. Lindemann , M. Lindner , J. A. M. Lopes , K. Lung , T. Marrodan Undagoitia , F. V. Massoli , A. J. Melgarejo Fernandez , Y. Meng , A. Molinario , E. Nativ , K. Ni , U. Oberlack , S. E. A. Orrigo , E. Pantic , R. Persiani , G. Plante , N. Priel , A. Rizzo , S. Rosendahl , J. M. F. dos Santos , G. Sartorelli , J. Schreiner , M. Schumann , L. Scotto Lavina , P. R. Scovell , M. Selvi , P. Shagin , H. Simgen , A. Teymourian , D. Thers , O. Vitells , H. Wang , M. Weber , C. Weinheimer

Dark matter sensitivity of multi-ton liquid xenon detectors

We study the sensitivity of multi ton-scale time projection chambers using a liquid xenon target, e.g., the proposed DARWIN instrument, to spin-independent and spin-dependent WIMP-nucleon scattering interactions. Taking into account…

Instrumentation and Detectors · Physics 2015-10-14 Marc Schumann , Laura Baudis , Lukas Bütikofer , Alexander Kish , Marco Selvi

Limits on spin-dependent WIMP-nucleon cross-sections from the XENON10 experiment

XENON10 is an experiment to directly detect weakly interacting massive particle (WIMPs), which may comprise the bulk of the non-baryonic dark matter in our Universe. We report new results for spin-dependent WIMP-nucleon interactions with…

Astrophysics · Physics 2019-08-14 J. Angle , E. Aprile , F. Arneodo , L. Baudis , A. Bernstein , A. Bolozdynya , P. Brusov , L. C. C. Coelho , C. E. Dahl , L. DeViveiros , A. D. Ferella , L. M. P. Fernandes , S. Fiorucci , R. J. Gaitskell , K. L. Giboni , R. Gomez , R. Hasty , L. Kastens , J. Kwong , J. A. M. Lopes , N. Madden , A. Manalaysay , A. Manzur , D. N. McKinsey , M. E. Monzani , K. Ni , U. Oberlack , J. Orboeck , G. Plante , R. Santorelli , J. M. F. dos Santos , P. Shagin , T. Shutt , P. Sorensen , S. Schulte , C. Winant , M. Yamashita

Searching for Heavy Dark Matter near the Planck Mass with XENON1T

Multiple viable theoretical models predict heavy dark matter particles with a mass close to the Planck mass, a range relatively unexplored by current experimental measurements. We use 219.4 days of data collected with the XENON1T experiment…

High Energy Physics - Experiment · Physics 2023-07-06 E. Aprile , K. Abe , S. Ahmed Maouloud , L. Althueser , B. Andrieu , E. Angelino , J. R. Angevaare , V. C. Antochi , D. Antón Martin , F. Arneodo , L. Baudis , A. L. Baxter , M. Bazyk , L. Bellagamba , R. Biondi , A. Bismark , E. J. Brookes , A. Brown , S. Bruenner , G. Bruno , R. Budnik , T. K. Bui , C. Cai , J. M. R. Cardoso , D. Cichon , A. P. Cimental Chavez , M. Clark , A. P. Colijn , J. Conrad , J. J. Cuenca-García , J. P. Cussonneau , V. D'Andrea , M. P. Decowski , P. Di Gangi , S. Di Pede , S. Diglio , K. Eitel , A. Elykov , S. Farrell , A. D. Ferella , C. Ferrari , H. Fischer , M. Flierman , W. Fulgione , C. Fuselli , P. Gaemers , R. Gaior , A. Gallo Rosso , M. Galloway , F. Gao , R. Glade-Beucke , L. Grandi , J. Grigat , H. Guan , M. Guida , R. Hammann , A. Higuera , C. Hils , L. Hoetzsch , N. F. Hood , J. Howlett , M. Iacovacci , Y. Itow , J. Jakob , F. Joerg , A. Joy , N. Kato , M. Kara , P. Kavrigin , S. Kazama , M. Kobayashi , G. Koltman , A. Kopec , F. Kuger , H. Landsman , R. F. Lang , L. Levinson , I. Li , S. Li , S. Liang , S. Lindemann , M. Lindner , K. Liu , J. Loizeau , F. Lombardi , J. Long , J. A. M. Lopes , Y. Ma , C. Macolino , J. Mahlstedt , A. Mancuso , L. Manenti , F. Marignetti , T. Marrodán Undagoitia , K. Martens , J. Masbou , D. Masson , E. Masson , S. Mastroianni , M. Messina , K. Miuchi , K. Mizukoshi , A. Molinario , S. Moriyama , K. Morå , Y. Mosbacher , M. Murra , J. Müller , K. Ni , U. Oberlack , B. Paetsch , J. Palacio , Q. Pellegrini , R. Peres , C. Peters , J. Pienaar , M. Pierre , V. Pizzella , G. Plante , T. R. Pollmann , J. Qi , J. Qin , D. Ramírez García , R. Singh , L. Sanchez , J. M. F. dos Santos , I. Sarnoff , G. Sartorelli , J. Schreiner , D. Schulte , P. Schulte , H. Schulze Eißing , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , S. Shi , E. Shockley , M. Silva , H. Simgen , A. Takeda , P. -L. Tan , A. Terliuk , D. Thers , F. Toschi , G. Trinchero , C. Tunnell , F. Tönnies , K. Valerius , G. Volta , C. Weinheimer , M. Weiss , D. Wenz , C. Wittweg , T. Wolf , V. H. S. Wu , Y. Xing , D. Xu , Z. Xu , M. Yamashita , L. Yang , J. Ye , L. Yuan , G. Zavattini , M. Zhong , T. Zhu

Search for bosonic superweakly interacting massive dark matter particles with the XMASS-I detector

Bosonic superweakly interacting massive particles (super-WIMPs) are a candidate for warm dark matter. With the absorption of such a boson by a xenon atom these dark matter candidates would deposit an energy equivalent to their rest mass in…

Cosmology and Nongalactic Astrophysics · Physics 2014-09-22 K. Abe , K. Hieda , K. Hiraide , S. Hirano , Y. Kishimoto , K. Ichimura , K. Kobayashi , S. Moriyama , K. Nakagawa , M. Nakahata , H. Ogawa , N. Oka , H. Sekiya , A. Shinozaki , Y. Suzuki , A. Takeda , O. Takachio , D. Umemoto , M. Yamashita , B. S. Yang , S. Tasaka , J. Liu , K. Martens , K. Hosokawa , K. Miuchi , A. Murata , Y. Onishi , Y. Otsuka , Y. Takeuchi , Y. H. Kim , K. B. Lee , M. K. Lee , J. S. Lee , Y. Fukuda , Y. Itow , K. Masuda , H. Takiya , H. Uchida , N. Y. Kim , Y. D. Kim , F. Kusaba , K. Nishijima , K. Fujii , I. Murayama , S. Nakamura

Direct Detection Constraints on Dark Photon Dark Matter

Dark matter detectors built primarily to probe elastic scattering of WIMPs on nuclei are also precise probes of light, weakly coupled particles that may be absorbed by the detector material. In this paper, we derive constraints on the…

High Energy Physics - Phenomenology · Physics 2015-07-23 Haipeng An , Maxim Pospelov , Josef Pradler , Adam Ritz

A dark matter WIMP that can be detected and definitively identified with currently planned experiments

A recently proposed dark matter WIMP has only second-order couplings to gauge bosons and itself. As a result, it has small annihilation, scattering, and creation cross-sections, and is consequently consistent with all current experiments…

High Energy Physics - Phenomenology · Physics 2021-08-02 Caden LaFontaine , Bailey Tallman , Spencer Ellis , Trevor Croteau , Brandon Torres , Sabrina Hernandez , Diego Cristancho Guerrero , Jessica Jaksik , Drue Lubanski , Roland E. Allen

Determining the WIMP mass using the complementarity between direct and indirect searches and the ILC

We study the possibility of identifying dark matter properties from XENON-like 100 kg experiments and the GLAST satellite mission. We show that whereas direct detection experiments will probe efficiently light WIMPs, given a positive…

High Energy Physics - Phenomenology · Physics 2009-02-09 N. Bernal , A. Goudelis , Y. Mambrini , C. Munoz

Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX data

We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including $1.4\times10^{4}\;\mathrm{kg\; day}$ of search exposure. This new…

Cosmology and Nongalactic Astrophysics · Physics 2016-05-17 LUX Collaboration , D. S. Akerib , H. M. Araújo , X. Bai , A. J. Bailey , J. Balajthy , P. Beltrame , E. P. Bernard , A. Bernstein , T. P. Biesiadzinski , E. M. Boulton , A. Bradley , R. Bramante , S. B. Cahn , M. C. Carmona-Benitez , C. Chan , J. J. Chapman , A. A. Chiller , C. Chiller , A. Currie , J. E. Cutter , T. J. R. Davison , L. de Viveiros , A. Dobi , J. E. Y. Dobson , E. Druszkiewicz , B. N. Edwards , C. H. Faham , S. Fiorucci , R. J. Gaitskell , V. M. Gehman , C. Ghag , K. R. Gibson , M. G. D. Gilchriese , C. R. Hall , M. Hanhardt , S. J. Haselschwardt , S. A. Hertel , D. P. Hogan , M. Horn , D. Q. Huang , C. M. Ignarra , M. Ihm , R. G. Jacobsen , W. Ji , K. Kazkaz , D. Khaitan , R. Knoche , N. A. Larsen , C. Lee , B. G. Lenardo , K. T. Lesko , A. Lindote , M. I. Lopes , D. C. Malling , A. Manalaysay , R. L. Mannino , M. F. Marzioni , D. N. McKinsey , D. M. Mei , J. Mock , M. Moongweluwan , J. A. Morad , A. St. J. Murphy , C. Nehrkorn , H. N. Nelson , F. Neves , K. O`Sullivan , K. C. Oliver-Mallory , R. A. Ott , K. J. Palladino , M. Pangilinan , E. K. Pease , P. Phelps , L. Reichhart , C. Rhyne , S. Shaw , T. A. Shutt , C. Silva , V. N. Solovov , P. Sorensen , S. Stephenson , T. J. Sumner , M. Szydagis , D. J. Taylor , W. Taylor , B. P. Tennyson , P. A. Terman , D. R. Tiedt , W. H. To , M. Tripathi , L. Tvrznikova , S. Uvarov , J. R. Verbus , R. C. Webb , J. T. White , T. J. Whitis , M. S. Witherell , F. L. H. Wolfs , K. Yazdani , S. K. Young , C. Zhang

DARWIN/XLZD: a future xenon observatory for dark matter and other rare interactions

The DARWIN/XLZD experiment is a next-generation dark matter detector with a multi-ten-ton liquid xenon time projection chamber at its core. Its principal goal will be to explore the experimentally accessible parameter space for Weakly…

Instrumentation and Methods for Astrophysics · Physics 2024-05-01 Laura Baudis

Low-mass dark matter search results from full exposure of PandaX-I experiment

We report the results of a weakly-interacting massive particle (WIMP) dark matter search using the full 80.1\;live-day exposure of the first stage of the PandaX experiment (PandaX-I) located in the China Jin-Ping Underground Laboratory. The…

High Energy Physics - Experiment · Physics 2015-09-23 PandaX Collaboration , Xiang Xiao , Xun Chen , Andi Tan , Yunhua Chen , Xiangyi Cui , Deqing Fang , Changbo Fu , Karl L. Giboni , Haowei Gong , Guodong Guo , Ming He , Xiangdong Ji , Yonglin Ju , Siao Lei , Shaoli Li , Qing Lin , Huaxuan Liu , Jianglai Liu , Xiang Liu , Wolfgang Lorenzon , Yugang Ma , Yajun Mao , Kaixuan Ni , Kirill Pushkin , Xiangxiang Ren , Michael Schubnell , Manbin Shen , Yuji Shi , Scott Stephenson , Hongwei Wang , Jiming Wang , Meng Wang , Siguang Wang , Xuming Wang , Zhou Wang , Shiyong Wu , Mengjiao Xiao , Pengwei Xie , Binbin Yan , Yinghui You , Xionghui Zeng , Tao Zhang , Li Zhao , Xiaopeng Zhou , Zhonghua Zhu

Potential for definitive discovery of a 70 GeV dark matter WIMP with only second-order gauge couplings

As astronomical observations and their interpretation improve, the case for cold dark matter (CDM) becomes increasingly persuasive. A particularly appealing version of CDM is a weakly interacting massive particle (WIMP) with a mass near the…

High Energy Physics - Phenomenology · Physics 2022-10-28 Bailey Tallman , Alexandra Boone , Adhithya Vijayakumar , Fiona Lopez , Samuel Apata , Jehu Martinez , Roland Allen

Radiogenic and Muon-Induced Backgrounds in the LUX Dark Matter Detector

The Large Underground Xenon (LUX) dark matter experiment aims to detect rare low-energy interactions from Weakly Interacting Massive Particles (WIMPs). The radiogenic backgrounds in the LUX detector have been measured and compared with…

Instrumentation and Methods for Astrophysics · Physics 2014-08-25 D. S. Akerib , H. M. Araujo , X. Bai , A. J. Bailey , J. Balajthy , E. Bernard , A. Bernstein , A. Bradley , D. Byram , S. B. Cahn , M. C. Carmona-Benitez , C. Chan , J. J. Chapman , A. A. Chiller , C. Chiller , T. Coffey , A. Currie , L. de Viveiros , A. Dobi , J. Dobson , E. Druszkiewicz , B. Edwards , C. H. Faham , S. Fiorucci , C. Flores , R. J. Gaitskell , V. M. Gehman , C. Ghag , K. R. Gibson , M. G. D. Gilchriese , C. Hall , S. A. Hertel , M. Horn , D. Q. Huang , M. Ihm , R. G. Jacobsen , K. Kazkaz , R. Knoche , N. A. Larsen , C. Lee , A. Lindote , M. I. Lopes , D. C. Malling , R. Mannino , D. N. McKinsey , D. -M. Mei , J. Mock , M. Moongweluwan , J. Morad , A. St. J. Murphy , C. Nehrkorn , H. Nelson , F. Neves , R. A. Ott , M. Pangilinan , P. D. Parker , E. K. Pease , K. Pech , P. Phelps , L. Reichhart , T. Shutt , C. Silva , V. N. Solovov , P. Sorensen , K. O'Sullivan , T. J. Sumner , M. Szydagis , D. Taylor , B. Tennyson , D. R. Tiedt , M. Tripathi , S. Uvarov , J. R. Verbus , N. Walsh , R. Webb , J. T. White , M. S. Witherell , F. L. H. Wolfs , M. Woods , C. Zhang

Direct Detection Limits on Heavy Dark Matter

Multiply-interacting massive particles (MIMPs) are heavy (>10^10 GeV/c^2) dark matter particles that interact strongly with regular matter, but may have evaded detection due to the low number density required to make up the local dark…

High Energy Physics - Phenomenology · Physics 2022-01-12 Michael Clark , Amanda Depoian , Bahaa Elshimy , Abigail Kopec , Rafael F. Lang , Shengchao Li , Juehang Qin

Search for Bosonic Super-WIMP Interactions with the XENON100 Experiment

We present results of searches for vector and pseudo-scalar bosonic super-WIMPs, which are dark matter candidates with masses at the keV-scale, with the XENON100 experiment. XENON100 is a dual-phase xenon time projection chamber operated at…

Cosmology and Nongalactic Astrophysics · Physics 2017-12-13 XENON collaboration , E. Aprile , J. Aalbers , F. Agostini , M. Alfonsi , L. Althueser , 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 , Bütikofer , J. Calven , C. Capelli , J. M. R. Cardoso , 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 , C. Geis , L. W. Goetzke , 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. Maris , 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 , D. Ramírez García , L. Rauch , S. Reichard , C. Reuter , A. Rizzo , 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 , Z. Wang , Y. Wei , C. Weinheimer , C. Wittweg , J. Wulf , J. Ye , Y. Zhang , T. Zhu