C
C. Levy
Researcher at University of Münster
Publications - 49
Citations - 6035
C. Levy is an academic researcher from University of Münster. The author has contributed to research in topics: Dark matter & WIMP. The author has an hindex of 27, co-authored 45 publications receiving 5566 citations. Previous affiliations of C. Levy include University at Albany, SUNY & Queen's University.
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Journal ArticleDOI
Xenon Bubble Chambers for Direct Dark Matter Detection
TL;DR: In this article, a new type of dark matter detector is proposed, a xenon bubble chamber, which combines the strengths of liquid xenon TPCs, namely event by event energy resolution, with those of a bubble chamber.
Journal ArticleDOI
Xenon Bubble Chambers for Direct Dark Matter Detection
TL;DR: In this article, a new type of dark matter detector is proposed, a xenon bubble chamber, which combines the strengths of liquid xenon TPCs, namely event by event energy resolution, with those of a bubble chamber.
Proceedings ArticleDOI
Optimization of Neutron Shielding for the PICASSO Experiment
S. Archambault,F. Aubin,M. Auger,E. Behnke,B. Beltran,B. Biskup,Karl J. Clark,X. Dai,A. Davour,J. Farine,M. H. Genest,G. Giroux,R. Gornea,R. Faust,C. B. Krauss,I. Lawson,Claude Leroy,C. Levy,L. Lessard,Ilan Levine,J. P. Martin,S. Kumaratunga,R. MacDonald,P. Nadeau,A. J. Noble,M.-C. Piro,Stanislav Pospisil,T. Shepherd,J. Sodomka,N. Starinski,I. Stekl,C. Storey,U. Wichoski,V. Zacek +33 more
TL;DR: In this article, different types of neutron shielding (water, polyethylene, borated water and polyethylenes doped with different compounds of boron and lithium) were compared from the point of view of neutron suppression as well as number of newly born y−rays.
Posted ContentDOI
Comment on "On the subtleties of searching for dark matter with liquid xenon detectors"
Elena Aprile,M. Alfonsi,K. Arisaka,F. Arneodo,C. Balan,Laura Baudis,Boris Bauermeister,A. Behrens,P. Beltrame,K. Bokeloh,Ethan Brown,Giacomo Bruno,R. Budnik,João Cardoso,W. T. Chen,B. Choi,David B. Cline,A. P. Colijn,H. Contreras,Jean-Pierre Cussonneau,M. P. Decowski,Ehud Duchovni,S. Fattori,A. D. Ferella,W. Fulgione,F. Gao,M. Garbini,C. Ghag,Karl Giboni,Luke Goetzke,C. Grignon,E. K. U. Gross,W. Hampel,Florian Kaether,A. Kish,J. Lamblin,H. Landsman,R. F. Lang,M. Le Calloch,C. Levy,K. E. Lim,Qing Lin,Sebastian Lindemann,Manfred Lindner,J.A.M. Lopes,K. Lung,Teresa Marrodán Undagoitia,F. V. Massoli,A. J. Melgarejo Fernandez,Y. Meng,A. Molinario,E. Nativ,Kaixuan Ni,U. Oberlack,S. E. A. Orrigo,E. Pantic,R. Persiani,Guillaume Plante,N. Priel,A. Rizzo,S. Rosendahl,J.M.F. dos Santos,G. Sartorelli,Jochen Schreiner,Marc Schumann,L. Scotto Lavina,P. R. Scovell,M. Selvi,P. Shagin,Hardy Simgen,A. Teymourian,D. Thers,O. Vitells,Hulin Wang,M. Weber,C. Weinheimer +75 more
TL;DR: In this article, Sorensen et al. pointed out the rationale for not considering the described effect in their final analysis and list several potential problems with his study, and pointed out that XENON100's upper limits on spin-independent WIMP-nucleon cross-sections for masses below 10 GeV may be understated by one order of magnitude or more.
Journal ArticleDOI
Background determination for the LUX-ZEPLIN dark matter experiment
Jelle Aalbers,D. S. Akerib,A. Musalhi,F. I. Alder,S. Alsum,CS Amarasinghe,A. Ames,Todd J. Anderson,N. Angelides,Henrique Araujo,J. E. Armstrong,M. Arthurs,A. Baker,J. Bang,J. Bargemann,A. Baxter,Kevin J. Beattie,P. Beltrame,Ethan Bernard,Ahmed F. Bhatti,Andreas Biekert,T. P. Biesiadzinski,H. J. Birch,G. M. Blockinger,B. Boxer,Charl Anne Brew,P. Br'as,Sergey Burdin,M. Buuck,R. Cabrita,M. C. Carmona-Benitez,C. Chan,A Chawla,H. Chen,Amity Chiang,N. Chott,Mark Converse,A. Cottle,G. A. Cox,Oisín Creaner,C. E. Dahl,A. David,Sucharita Dey,L. de Viveiros,Chuck Ding,J. E. Y. Dobson,E. Druszkiewicz,Stine Risdal Eriksen,A. Fan,N. M. Fearon,S. Fiorucci,H. U. Flaecher,E. D. Fraser,Thomas Fruth,R. J. Gaitskell,J. Genovesi,C. Ghag,Rachel M. Gibbons,M. G. D. Gilchriese,S. Gokhale,Jeffrey G. Green,M. G. D. van der Grinten,Chris Gwilliam,C. R. Hall,S. J. Han,Ellen Hartigan-O'Connor,S. J. Haselschwardt,S. A. Hertel,G. Heuermann,M. Horn,D. Q. Huang,Diana Hunt,C. M. Ignarra,R. G. Jacobsen,O. Jahangir,Robert S. Jampel,A. C. Kaboth,A. Kamaha,D. Khaitan,I. Khurana,Renee Kirk,D. Kodroff,L. Korley,Elena Korolkova,H. Kraus,S. Kravitz,L. Kreczko,Benjamin Krikler,V. A. Kudryavtsev,E. Leason,J. Lee,F. Leonard,K. T. Lesko,C. Levy,J. Lin,A. Lindote,R. Linehan,W. H. Lippincott,X. Liu,M.I. Lopes,E. Lopez Asamar,B. Lopez Paredes,Wolfgang Lorenzon,C Lu,S. Luitz,Peter Majewski,A. Manalaysay,R. L. Mannino,N. Marangou,Michael E. McCarthy,Daniel McKinsey,J. B. McLaughlin,Eric L. Miller,E. Mizrachi,A. Monte,M. E. Monzani,J. D. Morales Mendoza,E. C. Morrison,B. J. Mount,Matthew Murdy,A. St. J. Murphy,D. Naim,A. Naylor,Christopher Nedlik,H. N. Nelson,F. Neves,Alex Nguyen,J. A. Nikoleyczik,I. Olcina,K. C. Oliver-Mallory,James Edward Orpwood,K. J. Palladino,John Palmer,Nishat Parveen,S. J. Patton,Bjoern Penning,G. Pereira,Earl Perry,T. Pershing,A. Piepke,David Porzio,S. S. Poudel,Y. Qie,J. Reichenbacher,C. Rhyne,Q. Riffard,G. R. C. Rischbieter,Harjoat Riyat,Richard Rose,Patrick Rossiter,T.G.A. Rushton,D. Santone,A. B.M.R. Sazzad,R. W. Schnee,S. Shaw,T. A. Shutt,J.J. Silk,C. Silva,G. Sinev,R. Smith,M. Solmaz,V. N. Solovov,P. Sorensen,Jeremy Soria,I. Stancu,Amy Stevens,K. Stifter,B. Suerfu,T. J. Sumner,Neil Swanson,Matthew Szydagis,R. Taylor,W. C. Taylor,D. Temples,P. A. Terman,D. R. Tiedt,M. Timalsina,Zhong‐Fang Tong,Daniel Tovey,Joanne Neal Tranter,M.J. Trask,Mallika Tripathi,D. R. Tronstad,W. Turner,U. Utku,Antanas Vaitkus,A. Wang,W. Wang,Y. Wang,Jacob Ross Watson,R. C. Webb,T. J. Whitis,M. Williams,F.L.H. Wolfs,Susan Woodford,D. Woodward,Carly Jayne Wright,Qianxu Xia,X. Xiang,J Xu,Melody Yeh +200 more
TL;DR: The LUX-ZEPLIN experiment recently reported limits on WIMP-nucleus interactions from its initial science run, down to $9.2\times10^{-48}$ cm$^2$ for the spin-independent interaction of a 36 GeV/c$1.5 )-WIMP at 90% confidence level as discussed by the authors .