F
Florian Kaether
Researcher at Max Planck Society
Publications - 50
Citations - 7322
Florian Kaether is an academic researcher from Max Planck Society. The author has contributed to research in topics: CHOOZ & Dark matter. The author has an hindex of 29, co-authored 49 publications receiving 6900 citations.
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Journal ArticleDOI
Dark Matter Results from 225 Live Days of XENON100 Data
Elena Aprile,M. Alfonsi,K. Arisaka,F. Arneodo,C. Balan,Laura Baudis,Boris Bauermeister,A. Behrens,P. Beltrame,K. Bokeloh,Ethan Brown,Giacomo Bruno,Ran Budnik,João Cardoso,W. T. Chen,B. Choi,David B. Cline,Auke-Pieter Colijn,H. Contreras,Jean-Pierre Cussonneau,M. P. Decowski,Ehud Duchovni,S. Fattori,A. D. Ferella,W. Fulgione,F. Gao,M. Garbini,C. Ghag,K. L. Giboni,Luke Goetzke,C. Grignon,Eilam Gross,W. Hampel,Florian Kaether,A. Kish,J. Lamblin,H. Landsman,R. F. Lang,R. F. Lang,M. Le Calloch,C. Levy,K. E. Lim,Qing Lin,Sebastian Lindemann,Manfred Lindner,J. A. M. Lopes,K. Lung,T. Marrodán Undagoitia,F. V. Massoli,A. J. Melgarejo Fernandez,Y. Meng,A. Molinario,E. Nativ,Kaixuan Ni,Uwe Oberlack,Uwe Oberlack,S. E. A. Orrigo,E. Pantic,R. Persiani,G. 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,Hui Wang,M. Weber,Ch. Weinheimer +77 more
TL;DR: A search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso for 13 months during 2011 and 2012, has yielded no evidence for dark matter interactions.
Journal ArticleDOI
Indication of Reactor ν¯e Disappearance in the Double Chooz Experiment
Yoshio Abe,C. Aberle,T. Akiri,J. C. dos Anjos,F. Ardellier,A. F. Barbosa,A. Baxter,M. Bergevin,A. Bernstein,T.J.C. Bezerra,L. Bezrukhov,E. Blucher,M. Bongrand,Nathaniel Bowden,Christian Buck,J. Busenitz,Anatael Cabrera,E. Caden,L. Camilleri,R. Carr,M. Cerrada,P.-J. Chang,P. Chimenti,T. Classen,T. Classen,Antoine Collin,E. Conover,Janet Conrad,S. Cormon,J. I. Crespo-Anadón,M. Cribier,K. Crum,A. Cucoanes,M. V. d'Agostino,E. Damon,J.V. Dawson,Steven Dazeley,M. Dierckxsens,D. Dietrich,Z. Djurcic,M. Dracos,V. Durand,Yu. Efremenko,M. Elnimr,Y. Endo,A.V. Etenko,E. Falk,Muriel Fallot,M. Fechner,F. von Feilitzsch,J. Felde,S. M. Fernandes,D. Franco,A. J. Franke,M. Franke,H. Furuta,R. Gama,I. Gil-Botella,Lydie Giot,M. Göger-Neff,Luis González,M. C. Goodman,J. Tm. Goon,D. Greiner,B. Guillon,N. Haag,Caren Hagner,T. Hara,F. X. Hartmann,J. Hartnell,T. Haruna,J. Haser,A. Hatzikoutelis,T. Hayakawa,Michael Hofmann,G. A. Horton-Smith,Masaki Ishitsuka,J. Jochum,C. Jollet,C. L. Jones,Florian Kaether,L.N. Kalousis,Yuri Kamyshkov,Daniel M. Kaplan,T. Kawasaki,G. Keefer,E. Kemp,H. de Kerret,Y. Kibe,T. Konno,D. Kryn,M. Kuze,Tobias Lachenmaier,C. E. Lane,C. Langbrandtner,Thierry Lasserre,Alain Letourneau,David Lhuillier,H. P. Lima,Manfred Lindner,Yehan Liu,J. M. López-Castanõ,J. M. LoSecco,Bayarto Lubsandorzhiev,S. Lucht,D. Mckee,D. Mckee,J. Maeda,C. N. Maesano,C. Mariani,J. Maricic,J. Martino,T. Matsubara,G. Mention,A. Meregaglia,T. Miletic,R. Milincic,A. Milzstajn,H. Miyata,D. Motta,Th. A. Mueller,Yasushi Nagasaka,K. Nakajima,P. Novella,M. Obolensky,Lothar Oberauer,A. Onillon,A. Osborn,I. Ostrovskiy,C. Palomares,S. J. M. Peeters,I. M. Pepe,S. Perasso,P. Perrin,P. Pfahler,Amanda Porta,W. Potzel,R. Queval,J. Reichenbacher,B. Reinhold,A. Remoto,A. Remoto,D. E. Reyna,M. Röhling,S. Roth,H. A. Rubin,Y. Sakamoto,R. Santorelli,F. Sato,S. Schönert,Stefan Schoppmann,U. Schwan,Thomas Schwetz,M. H. Shaevitz,D. Shrestha,J. L. Sida,V. V. Sinev,M. D. Skorokhvatov,E. Smith,J. Spitz,A. Stahl,I. Stancu,Matthew L Strait,A. Stüken,F. Suekane,S. V. Sukhotin,T. Sumiyoshi,Ying Sun,Z. Sun,R. Svoboda,H. Tabata,N. Tamura,Kazuhiro Terao,A. Tonazzo,M. Toups,H. H. Trinh Thi,C. Veyssiere,Sebastian Wagner,H. Watanabe,B. White,Christopher Wiebusch,Lindley Winslow,M. Worcester,Michael Wurm,E. Yanovitch,F. Yermia,K. Zbiri,K. Zbiri,V. Zimmer +188 more
TL;DR: The Double Chooz experiment presents an indication of reactor electron antineutrino disappearance consistent with neutrino oscillations, and an observed-to-predicted ratio of events of 0.944±0.016 and a deficit can be interpreted as a nonzero value of the still unmeasured neutrinos mixing parameter sin(2)2θ(13).
Journal ArticleDOI
Physics reach of the XENON1T dark matter experiment
Elena Aprile,Jelle Aalbers,F. Agostini,M. Alfonsi,F. D. Amaro,M. Anthony,Lior Arazi,F. Arneodo,C. Balan,P. Barrow,Laura Baudis,Boris Bauermeister,Boris Bauermeister,T. Berger,P. A. Breur,Amos Breskin,April S. Brown,Ethan Brown,S. Bruenner,Giacomo Bruno,Ran Budnik,L. Bütikofer,João Cardoso,M. Cervantes,D. Cichon,D. Coderre,Auke-Pieter Colijn,Jan Conrad,H. Contreras,Jean-Pierre 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,Michelle Galloway,M. Garbini,C. Geis,Luke Goetzke,Z. Greene,C. Grignon,E. K. U. Gross,W. Hampel,C. Hasterok,R. Itay,Florian Kaether,B. Kaminsky,G. Kessler,A. Kish,H. Landsman,R. F. Lang,D. Lellouch,L. Levinson,M. Le Calloch,C. Levy,Sebastian Lindemann,Manfred Lindner,J. A. M. Lopes,A. Lyashenko,S. Macmullin,A. Manfredini,T. Marrodán Undagoitia,Julien Masbou,F. V. Massoli,D. Mayani,A. J. Melgarejo Fernandez,Y. Meng,M. Messina,K. Micheneau,B. Miguez,A. Molinario,M. Murra,J. Naganoma,Uwe Oberlack,S. E. A. Orrigo,P. Pakarha,Bart Pelssers,R. Persiani,F. Piastra,J. Pienaar,Guillaume Plante,N. Priel,L. Rauch,S. Reichard,C. Reuter,A. Rizzo,S. Rosendahl,N. Rupp,J.M.F. dos Santos,Gabriella Sartorelli,M. Scheibelhut,S. Schindler,Jochen Schreiner,Marc Schumann,L. Scotto Lavina,M. Selvi,P. Shagin,Hardy Simgen,A. Stein,D. Thers,A. Tiseni,G. C. Trinchero,C. Tunnell,M. von Sivers,R. Wall,Hui Wang,M. Weber,Yuehuan Wei,Ch. Weinheimer,J. Wulf,Yanxi Zhang +115 more
TL;DR: In this article, the expected sensitivity of the Xenon1T experiment to the spin-independent WIMP-nucleon interaction cross section was investigated based on Monte Carlo predictions of the electronic and nuclear recoil backgrounds.
Journal ArticleDOI
Reanalysis of the GALLEX solar neutrino flux and source experiments
TL;DR: In this paper, the authors retrospectively updated the Gallex results with the help of new technical data that were impossible to acquire for principle reasons before the completion of the low rate measurement phase (that is, before the end of the GNO solar runs).
Journal ArticleDOI
Complete results for five years of GNO solar neutrino observations
M. Altmann,M. Balata,P. Belli,E. Bellotti,R. Bernabei,E. Burkert,C. Cattadori,R. Cerulli,Marco Chiarini,M. Cribier,S. d'Angelo,G. Del Re,K.H. Ebert,F. von Feilitzsch,N. Ferrari,W. Hampel,F. Hartmann,E. Henrich,G. Heusser,Florian Kaether,J. Kiko,Till Kirsten,T. Lachenmaier,J.-C. Lanfranchi,Matthias Laubenstein,Klaus Lützenkirchen,Klaus Mayer,P. Moegel,D. Motta,Stefano Nisi,J. Oehm,Luciano Pandola,F. Petricca,W. Potzel,H. Richter,S. Schoenert,Maria Wallenius,Marcin Wójcik,L. Zanotti +38 more
TL;DR: In this article, the authors report the complete GNO solar neutrino results for the measuring periods GNO, III, GNO II, and GNO I. The GNO experiment is now terminated after altogether 58 solar exposure runs that were performed between 20 May 1998 and 9 April 2003.