H
Henrique Araujo
Researcher at Imperial College London
Publications - 161
Citations - 36145
Henrique Araujo is an academic researcher from Imperial College London. The author has contributed to research in topics: Dark matter & Xenon. The author has an hindex of 43, co-authored 155 publications receiving 31255 citations. Previous affiliations of Henrique Araujo include Rutherford Appleton Laboratory.
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Journal ArticleDOI
Geant4—a simulation toolkit
S. Agostinelli,John Allison,K. Amako,J. Apostolakis,Henrique Araujo,P. Arce,Makoto Asai,D. Axen,S. Banerjee,G. Barrand,F. Behner,Lorenzo Bellagamba,J. Boudreau,L. Broglia,A. Brunengo,H. Burkhardt,Stephane Chauvie,J. Chuma,R. Chytracek,Gene Cooperman,G. Cosmo,P. V. Degtyarenko,Andrea Dell'Acqua,G. Depaola,D. Dietrich,R. Enami,A. Feliciello,C. Ferguson,H. Fesefeldt,Gunter Folger,Franca Foppiano,Alessandra Forti,S. Garelli,S. Gianì,R. Giannitrapani,D. Gibin,J. J. Gomez Y Cadenas,I. González,G. Gracia Abril,G. Greeniaus,Walter Greiner,Vladimir Grichine,A. Grossheim,Susanna Guatelli,P. Gumplinger,R. Hamatsu,K. Hashimoto,H. Hasui,A. Heikkinen,A. S. Howard,Vladimir Ivanchenko,A. Johnson,F.W. Jones,J. Kallenbach,Naoko Kanaya,M. Kawabata,Y. Kawabata,M. Kawaguti,S.R. Kelner,Paul R. C. Kent,A. Kimura,T. Kodama,R. P. Kokoulin,M. Kossov,Hisaya Kurashige,E. Lamanna,Tapio Lampén,V. Lara,Veronique Lefebure,F. Lei,M. Liendl,W. S. Lockman,Francesco Longo,S. Magni,M. Maire,E. Medernach,K. Minamimoto,P. Mora de Freitas,Yoshiyuki Morita,K. Murakami,M. Nagamatu,R. Nartallo,Petteri Nieminen,T. Nishimura,K. Ohtsubo,M. Okamura,S. W. O'Neale,Y. Oohata,K. Paech,J Perl,Andreas Pfeiffer,Maria Grazia Pia,F. Ranjard,A.M. Rybin,S.S Sadilov,E. Di Salvo,Giovanni Santin,Takashi Sasaki,N. Savvas,Y. Sawada,Stefan Scherer,S. Sei,V. Sirotenko,David J. Smith,N. Starkov,H. Stoecker,J. Sulkimo,M. Takahata,Satoshi Tanaka,E. Tcherniaev,E. Safai Tehrani,M. Tropeano,P. Truscott,H. Uno,L. Urbán,P. Urban,M. Verderi,A. Walkden,W. Wander,H. Weber,J.P. Wellisch,Torre Wenaus,D.C. Williams,Douglas Wright,T. Yamada,H. Yoshida,D. Zschiesche +126 more
TL;DR: The Gelfant 4 toolkit as discussed by the authors is a toolkit for simulating the passage of particles through matter, including a complete range of functionality including tracking, geometry, physics models and hits.
Journal ArticleDOI
Geant4 developments and applications
John Allison,K. Amako,John Apostolakis,Henrique Araujo,P.A. Dubois,Makoto Asai,G. Barrand,R. Capra,Stephane Chauvie,R Chytracek,G.A.P. Cirrone,Gene Cooperman,G. Cosmo,Giacomo Cuttone,G.G. Daquino,M. Donszelmann,M. Dressel,Gunter Folger,Franca Foppiano,J. Generowicz,Vladimir Grichine,Susanna Guatelli,P. Gumplinger,A. Heikkinen,Ivana Hrivnacova,A. S. Howard,Sebastien Incerti,Vladimir Ivanchenko,T. Johnson,F.W. Jones,Tatsumi Koi,R. P. Kokoulin,M. Kossov,Hisaya Kurashige,V. Lara,S.A. Larsson,Fan Lei,O. Link,Francesco Longo,M. Maire,A. Mantero,B. Mascialino,I. McLaren,Patricia Mendez Lorenzo,K. Minamimoto,K. Murakami,Petteri Nieminen,Luciano Pandola,S. Parlati,Luis Peralta,J Perl,Andreas Pfeiffer,Maria Grazia Pia,Alberto Ribon,Pedro Rodrigues,Giorgio Ivan Russo,S.S Sadilov,Giovanni Santin,Takashi Sasaki,David J. Smith,N. Starkov,Satoshi Tanaka,E. Tcherniaev,B. Tome,A. Trindade,Pete Truscott,L. Urbán,M. Verderi,A. Walkden,J.P. Wellisch,D.C. Williams,Douglas Wright,H. Yoshida +72 more
TL;DR: GeGeant4 as mentioned in this paper is a software toolkit for the simulation of the passage of particles through matter, it is used by a large number of experiments and projects in a variety of application domains, including high energy physics, astrophysics and space science, medical physics and radiation protection.
Journal ArticleDOI
First results from the LUX dark matter experiment at the Sanford Underground Research Facility
D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,S. Bedikian,Ethan Bernard,A. Bernstein,Alexander Bolozdynya,A. W. Bradley,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,J.J. Chapman,A. A. Chiller,C. Chiller,K. Clark,T. Coffey,A. Currie,A. Curioni,Steven Dazeley,L. de Viveiros,A. Dobi,J. E. Y. Dobson,E. M. Dragowsky,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. Fiorucci,C. E. Flores,R. J. Gaitskell,V. M. Gehman,C. Ghag,K.R. Gibson,Murdock Gilchriese,C. R. Hall,M. Hanhardt,S. A. Hertel,M. Horn,D. Q. Huang,M. Ihm,R. G. Jacobsen,L. Kastens,K. Kazkaz,R. Knoche,S. Kyre,R. L. Lander,N. A. Larsen,C. Lee,David Leonard,K. T. Lesko,A. Lindote,M.I. Lopes,A. Lyashenko,D.C. Malling,R. L. Mannino,Daniel McKinsey,Dongming Mei,J. Mock,M. Moongweluwan,J. A. Morad,M. Morii,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,James Nikkel,R. A. Ott,M. Pangilinan,P. D. Parker,E. K. Pease,K. Pech,P. Phelps,L. Reichhart,T. A. Shutt,C. Silva,W. Skulski,C. Sofka,V. N. Solovov,P. Sorensen,T.M. Stiegler,K. O'Sullivan,T. J. Sumner,Robert Svoboda,M. Sweany,Matthew Szydagis,D. J. Taylor,B. P. Tennyson,D. R. Tiedt,Mani Tripathi,S. Uvarov,J.R. Verbus,N. Walsh,R. C. Webb,J. T. White,D. White,M. S. Witherell,M. Wlasenko,F.L.H. Wolfs,M. Woods,Chao Zhang +101 more
TL;DR: The first WIMP search data set is reported, taken during the period from April to August 2013, presenting the analysis of 85.3 live days of data, finding that the LUX data are in disagreement with low-mass W IMP signal interpretations of the results from several recent direct detection experiments.
Journal ArticleDOI
Results from a Search for Dark Matter in the Complete LUX Exposure
D. S. Akerib,S. Alsum,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,R. Bramante,P. Brás,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,A.A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,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. Kamdin,K. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel 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,K. J. Palladino,E. K. Pease,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,T. A. Shutt,C. Silva,M. Solmaz,V. N. Solovov,P. Sorensen,S. Stephenson,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,Mani Tripathi,L. Tvrznikova,S. Uvarov,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,M. S. Witherell,F.L.H. Wolfs,Jilei Xu,K. Yazdani,Sarah Young,Chao Zhang +100 more
TL;DR: This search yields no evidence of WIMP nuclear recoils and constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×10^{4} kg day exposure of the Large Underground Xenon experiment are reported.
Journal ArticleDOI
Improved limits on scattering of weakly interacting massive particles from reanalysis of 2013 LUX data
D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,A. W. Bradley,R. Bramante,Sidney 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,Daniel 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,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,Mani 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,Sarah Young,Chao Zhang +100 more
TL;DR: This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV.