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The XMASS project aims to detect dark matter, pp and $^{7}$Be solar neutrinos, and neutrinoless double beta decay using ultra pure liquid xenon. The first phase of the XMASS experiment searches for dark matter. In this paper, we describe…

We study the sensitivity to the decay of a heavy neutral lepton into $e^+e^-$-pairs using the solar boron-8 neutrino flux as source. We provide a fully differential cross section for this process including the interference of neutral and…

High Energy Physics - Phenomenology · Physics 2025-06-05 Patrick Huber , Yulun Li

Large detectors employing xenon are a leading technology in existing and planned searches for new physics, including searches for neutrinoless double beta decay ($0\nu\beta\beta$) and dark matter. While upcoming detectors will employ target…

Dark matter detectors will soon be sensitive to Solar neutrinos via two distinct channels: coherent neutrino-nucleus scattering and neutrino electron elastic scattering. We establish an analysis method for extracting Solar model properties…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 J. Billard , L. Strigari , E. Figueroa-Feliciano

Neutrinoless double beta decays in liquid xenon produce a significant amount of Cherenkov light, with a photon number and angular distribution that distinguishes these events from common backgrounds. A GEANT4 simulation was used to simulate…

Instrumentation and Detectors · Physics 2019-02-20 Jason Philip Brodsky , Samuele Sangiorgio , Michael Heffner , Tyana Stiegler

We show that the Deep Underground Neutrino Experiment (DUNE), with significant but feasible new efforts, has the potential to deliver world-leading results in solar neutrinos. With a 100 kton-year exposure, DUNE could detect $\gtrsim 10^5$…

High Energy Physics - Phenomenology · Physics 2020-07-27 Francesco Capozzi , Shirley Weishi Li , Guanying Zhu , John F. Beacom

The projected sensitivity of the LUX-ZEPLIN (LZ) experiment to two-neutrino and neutrinoless double beta decay of $^{134}$Xe is presented. LZ is a 10-tonne xenon time projection chamber optimized for the detection of dark matter particles,…

Instrumentation and Detectors · Physics 2022-01-12 The LUX-ZEPLIN , Collaboration , : , D. S. Akerib , A. K. Al Musalhi , S. K. Alsum , C. S. Amarasinghe , A. Ames , T. J. Anderson , N. Angelides , H. M. Araujo , J. E. Armstrong , M. Arthurs , X. Bai , J. Balajthy , S. Balashov , J. Bang , J. W. Bargemann , D. Bauer , A. Baxter , P. Beltrame , E. P. Bernard , A. Bernstein , A. Bhatti , A. Biekert , T. P. Biesiadzinski , H. J. Birch , G. M. Blockinger , E. Bodnia , B. Boxer , C. A. J. Brew , P. Bras , S. Burdin , J. K. Busenitz , M. Buuck , R. Cabrita , M. C. Carmona-Benitez , M. Cascella , C. Chan , N. I. Chott , A. Cole , M. V. Converse , A. Cottle , G. Cox , O. Creaner , J. E. Cutter , C. E. Dahl , L. de Viveiros , J. E. Y. Dobson , E. Druszkiewicz , S. R. Eriksen , A. Fan , S. Fayer , N. M. Fearon , S. Fiorucci , H. Flaecher , E. D. Fraser , T. Fruth , R. J. Gaitskell , J. Genovesi , C. Ghag , E. Gibson , S. Gokhale , M. G. D. van der Grinten , C. B. Gwilliam , C. R. Hall , S. J. Haselschwardt , S. A. Hertel , M. Horn , D. Q. Huang , C. M. Ignarra , O. Jahangir , R. S. James , W. Ji , J. Johnson , A. C. Kaboth , A. C. Kamaha , K. Kamdin , K. Kazkaz , D. Khaitan , A. Khazov , I. Khurana , D. Kodroff , L. Korley , E. V. Korolkova , H. Kraus , S. Kravitz , L. Kreczko , B. Krikler , V. A. Kudryavtsev , E. A. Leason , J. Lee , D. S. Leonard , K. T. Lesko , C. Levy , J. Liao , J. Lin , A. Lindote , R. Linehan , W. H. Lippincott , X. Liu , M. I. Lopes , E. Lopez Asamar , B. Lopez Paredes , W. Lorenzon , S. Luitz , P. A. Majewski , A. Manalaysay , L. Manenti , R. L. Mannino , N. Marangou , M. E. McCarthy , D. N. McKinsey , J. McLaughlin , E. H. Miller , E. Mizrachi , A. Monte , M. E. Monzani , J. A. Morad , J. D. Morales Mendoza , E. Morrison , B. J. Mount , A. St. J. Murphy , D. Naim , A. Naylor , C. Nedlik , H. N. Nelson , F. Neves , J. A. Nikoleyczik , A. Nilima , I. Olcina , K. C. Oliver-Mallory , S. Pal , K. J. Palladino , J. Palmer , S. Patton , N. Parveen , E. K. Pease , B. Penning , G. Pereira , A. Piepke , Y. Qie , J. Reichenbacher , C. A. Rhyne , A. Richards , Q. Riffard , G. R. C. Rischbieter , R. Rosero , P. Rossiter , D. Santone , A. B. M. R. Sazzad , R. W. Schnee , P. R. Scovell , S. Shaw , T. A. Shutt , J. J. Silk , C. Silva , R. Smith , M. Solmaz , V. N. Solovov , P. Sorensen , J. Soria , I. Stancu , A. Stevens , K. Stifter , B. Suerfu , T. J. Sumner , N. Swanson , M. Szydagis , W. C. Taylor , R. Taylor , D. J. Temples , P. A. Terman , D. R. Tiedt , M. Timalsina , W. H. To , D. R. Tovey , M. Tripathi , D. R. Tronstad , W. Turner , U. Utku , A. Vaitkus , B. Wang , J. J. Wang , W. Wang , J. R. Watson , R. C. Webb , R. G. White , T. J. Whitis , M. Williams , F. L. H. Wolfs , D. Woodward , C. J. Wright , X. Xiang , J. Xu , M. Yeh , P. Zarzhitsky

The nEXO neutrinoless double beta decay experiment is designed to use a time projection chamber and 5000 kg of isotopically enriched liquid xenon to search for the decay in $^{136}$Xe. Progress in the detector design, paired with higher…

Nuclear Experiment · Physics 2022-02-24 nEXO Collaboration , G. Adhikari , S. Al Kharusi , E. Angelico , G. Anton , I. J. Arnquist , I. Badhrees , J. Bane , V. Belov , E. P. Bernard , T. Bhatta , A. Bolotnikov , P. A. Breur , J. P. Brodsky , E. Brown , T. Brunner , E. Caden , G. F. Cao , L. Cao , C. Chambers , B. Chana , S. A. Charlebois , D. Chernyak , M. Chiu , B. Cleveland , R. Collister , S. A. Czyz , J. Dalmasson , T. Daniels , L. Darroch , R. DeVoe , M. L. Di Vacri , J. Dilling , Y. Y. Ding , A. Dolgolenko , M. J. Dolinski , A. Dragone , J. Echevers , M. Elbeltagi , L. Fabris , D. Fairbank , W. Fairbank , J. Farine , S. Ferrara , S. Feyzbakhsh , Y. S. Fu , G. Gallina , P. Gautam , G. Giacomini , W. Gillis C. Gingras , D. Goeldi , R. Gornea , G. Gratta , C. A. Hardy , K. Harouaka , M. Heffner , E. W. Hoppe , A. House , A. Iverson , A. Jamil , M. Jewell , X. S. Jiang , A. Karelin , L. J. Kaufman , I. Kotov , R. Krücken , A. Kuchenkov , K. S. Kumar , Y. Lan , A. Larson , K. G. Leach , B. G. Lenardo , D. S. Leonard , G. Li , S. Li , Z. Li , C. Licciardi , R. Lindsay , R. MacLellan , M. Mahtab , P. Martel-Dion , J. Masbou , N. Massacret , T. McElroy , K. McMichael , M. Medina Peregrina , T. Michel , B. Mong , D. C. Moore , K. Murray , J. Nattress , C. R. Natzke , R. J. Newby , K. Ni , F. Nolet , O. Nusair , J. C. Nzobadila Ondze , K. Odgers , A. Odian , J. L. Orrell , G. S. Ortega , C. T. Overman , S. Parent , A. Perna , A. Piepke , A. Pocar , J-F. Pratte , N. Priel , V. Radeka , E. Raguzin , G. J. Ramonnye , T. Rao , H. Rasiwala , S. Rescia , F. Retière , J. Ringuette , V. Riot , T. Rossignol , P. C. Rowson , N. Roy , R. Saldanha , S. Sangiorgio , X. Shang , A. K. Soma , F. Spadoni , V. Stekhanov , X. L. Sun , M. Tarka , S. Thibado , A. Tidball , J. Todd , T. Totev , S. Triambak , R. H. M. Tsang , T. Tsang , F. Vachon , V. Veeraraghavan , S. Viel , C. Vivo-Vilches , P. Vogel , J-L. Vuilleumier , M. Wagenpfeil , T. Wager , M. Walent , K. Wamba , Q. Wang , W. Wei , L. J. Wen , U. Wichoski , S. Wilde , M. Worcester , S. X. Wu , W. H. Wu , X. Wu , Q. Xia , W. Yan , H. Yang , L. Yang , O. Zeldovich , J. Zhao , T. Ziegler

``Top--down'' models explain the observation of ultra high energy cosmic rays (UHECR; $E \gsim 5 \cdot 10^{19}$ eV) through the decay of very massive, long--lived ``$X$ particles''. If superparticles with masses near a TeV exist, $X$ decays…

High Energy Physics - Phenomenology · Physics 2008-11-26 Sascha Bornhauser , Manuel Drees

Searches for light sterile neutrinos are motivated by the unexpected observation of electron neutrino appearance in short-baseline experiments, such as the Liquid Scintillator Neutrino Detector (LSND) and the Mini Booster Neutrino…

High Energy Physics - Phenomenology · Physics 2021-11-08 Carlos A. Argüelles , Jordi Salvado

We discuss an alternative approach to the detection of solar neutrinos using a coarsely segmented detector based on inverse-beta decay onto $^{160}$Gd or $^{176}$Yb. While it is know that similar approaches, already discussed in the…

High Energy Physics - Experiment · Physics 2009-10-31 G. Gratta , Y. F. Wang

In the last years, liquid-scintillator detectors have opened a new window for the observation of low-energetic astrophysical neutrino sources. In 2007, the solar neutrino experiment Borexino began its data-taking in the Gran Sasso…

Large liquid scintillator detectors, such as JUNO, present a new opportunity to study neutral current events from the low-energy end of the atmospheric neutrinos, and possible new physics signals due to light dark matter. We carefully study…

High Energy Physics - Phenomenology · Physics 2022-12-06 Bhavesh Chauhan , Basudeb Dasgupta , Amol Dighe

The XENON1T experiment recently reported an excess of events at low electron recoil energies, which may be due to interactions of solar neutrinos inside the detector via a large neutrino magnetic moment. We point out that a $^{51}$Cr…

High Energy Physics - Phenomenology · Physics 2020-06-30 Pilar Coloma , Patrick Huber , Jonathan M. Link

Coherent elastic neutrino-nucleus scattering (CE$\nu$NS) poses an irreducible background in the search for dark matter-nucleus elastic scatterings, which is commonly known as the neutrino floor. As direct dark matter search experiments keep…

Dark matter (DM) direct detection experiments are entering the multiple-ton era and will be sensitive to the coherent elastic neutrino nucleus scattering (CE$\nu$NS) of solar neutrinos, enabling the possibility to explore contributions from…

High Energy Physics - Phenomenology · Physics 2022-03-29 Yu-Feng Li , Shuo-yu Xia

The background on double beta decay searches due to elastic electron scattering of solar neutrinos of all double beta emitters with Q-value larger than 2 MeV is calculated, taking into account survival probability and flux uncertainties of…

High Energy Physics - Phenomenology · Physics 2015-03-19 N. F. de Barros , K. Zuber

We present a technique for separating nuclear double beta decay ($\beta\beta$-decay) events from background neutrino interactions due to $^{8}$B decays in the sun. This background becomes dominant in a kiloton-scale liquid-scintillator…

Instrumentation and Detectors · Physics 2017-03-08 Andrey Elagin , Henry Frisch , Brian Naranjo , Jonathan Ouellet , Lindley Winslow , Taritree Wongjirad

Dual-phase liquid xenon (LXe) detectors lead the direct search for particle dark matter. Understanding the signal production process of nuclear recoils in LXe is essential for the interpretation of LXe based dark matter searches. Up to now,…

Instrumentation and Detectors · Physics 2018-12-12 Elena Aprile , Matthew Anthony , Qing Lin , Zach Greene , Patrick de Perio , Fei Gao , Joseph Howlett , Guillaume Plante , Yun Zhang , Tianyu Zhu

The PANDAX-4T and XENONnT experiments present indications of Coherent Elastic Neutrino Nucleus Scattering (CE$\nu$NS) from ${}^{8}$B solar neutrinos at 2.6$\sigma$ and 2.7$\sigma$, respectively. This constitutes the first observation of the…

High Energy Physics - Phenomenology · Physics 2025-08-04 Pablo Blanco-Mas , Pilar Coloma , Gonzalo Herrera , Patrick Huber , Joachim Kopp , Ian M. Shoemaker , Zahra Tabrizi