C. E. Dahl
Northwestern University
75 Papers
82 Citations
C. E. Dahl is an academic researcher from Northwestern University. The author has contributed to research in topics: Dark matter & Bubble chamber. The author has an hindex of 24, co-authored 48 publications. Previous affiliations of C. E. Dahl include Princeton University & Case Western Reserve University.
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Papers
First results from the XENON10 dark matter experiment at the gran sasso national laboratory
J. Angle,J. Angle,Elena Aprile,F. Arneodo,Laura Baudis,A. Bernstein,Alexander Bolozdynya,P. P. Brusov,Luis Coelho,C. E. Dahl,C. E. Dahl,L. DeViveiros,A. D. Ferella,L.M.P. Fernandes,S. Fiorucci,R. J. Gaitskell,Karl Giboni,R. Gomez,R. Hasty,L. Kastens,J. Kwong,J. Kwong,J. A. M. Lopes,N. Madden,A. Manalaysay,A. Manalaysay,A. Manzur,Daniel McKinsey,M. E. Monzani,Kaixuan Ni,Uwe Oberlack,J. Orboeck,Guillaume Plante,R. Santorelli,J.M.F. dos Santos,P. Shagin,T. A. Shutt,P. Sorensen,S. Schulte,C. Winant,Masaki Yamashita +40 more
TL;DR: A blind analysis of 58.6 live days of data excludes previously unexplored parameter space, setting a new 90% C.L. upper limit for the WIMP-nucleon spin-independent cross section of 8.8x10(-44) cm2 for a W IMP mass of 100 GeV/c2, which further constrains predictions of supersymmetric models.
Search for light dark matter in XENON10 data.
J. Angle,J. Angle,Elena Aprile,F. Arneodo,Laura Baudis,A. Bernstein,Alexander Bolozdynya,Luis Coelho,C. E. Dahl,L. DeViveiros,A. D. Ferella,L.M.P. Fernandes,S. Fiorucci,R. J. Gaitskell,Karl Giboni,R. Gomez,R. Hasty,L. Kastens,J. Kwong,J. A. M. Lopes,Norman W. Madden,A. Manalaysay,A. Manalaysay,A. Manzur,Daniel McKinsey,M. E. Monzani,Kaixuan Ni,Uwe Oberlack,Uwe Oberlack,J. Orboeck,Guillaume Plante,R. Santorelli,J.M.F. dos Santos,S. Schulte,P. Shagin,T. A. Shutt,P. Sorensen,C. Winant,Masaki Yamashita +38 more
TL;DR: The data strongly constrain recent elastic dark matter interpretations of excess low-energy events observed by CoGeNT and CRESST-II, as well as the DAMA annual modulation signal.
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Dark Matter Search Results from the PICO-2L C3F8 Bubble Chamber.
C. Amole,Miguel Ardid,David M. Asner,D. Baxter,E. Behnke,P. S. Bhattacharjee,H. Borsodi,M. Bou-Cabo,S. J. Brice,Daniel Broemmelsiek,K. Clark,J. I. Collar,P. S. Cooper,M. Crisler,C. E. Dahl,C. E. Dahl,S. Daley,Madhusmita Das,F. Debris,N. Dhungana,J. Farine,Ivan Felis,R. Filgas,M. Fines-Neuschild,Francoise Girard,G. Giroux,M. Hai,J. Hall,O. Harris,C. M. Jackson,M. Jin,C. B. Krauss,M. Lafrenière,M. Laurin,I. Lawson,I. Levine,W. H. Lippincott,E. Mann,J. P. Martin,Deepam Maurya,Pitam Mitra,R. Neilson,R. Neilson,A. J. Noble,A. Plante,R. B. Podviianiuk,Shashank Priya,A. E. Robinson,M. Ruschman,O. Scallon,O. Scallon,S. Seth,Andrew Sonnenschein,N. Starinski,I. Stekl,E. Vázquez-Jáuregui,E. Vázquez-Jáuregui,J. Wells,U. Wichoski,V. Zacek,Jie Zhang +60 more
TL;DR: These data provide the most sensitive direct detection constraints on WIMP-proton spin-dependent scattering to date, with significant sensitivity at low W IMP masses for spin-independent WIMp-nucleon scattering.
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First dark matter search results from a 4-kg CF$_3$I bubble chamber operated in a deep underground site
E. Behnke,J. Behnke,S. J. Brice,Daniel Broemmelsiek,J. I. Collar,A. Conner,P. S. Cooper,M. B. Crisler,C. E. Dahl,D. Fustin,E. Grace,J. Hall,M. Hu,I. Levine,W. H. Lippincott,T. Moan,T. Nania,E. J. Ramberg,A. E. Robinson,Andrew Sonnenschein,M. Szydagis,E. Vázquez-Jáuregui +21 more
TL;DR: In this article, the authors used ultrasound analysis to discriminate alpha decay background events from single nuclear recoils, with a lower bound of >99.3% rejection of alpha decay events.
Dark Matter Search Results from the PICO-60C(3)F(8) Bubble Chamber
C. Amole,M. Ardid,I. J. Arnquist,D. M. Asner,D. Baxter,E. Behnke,Pijushpani Bhattacharjee,H. Borsodi,Manuel Bou-Cabo,P. Campion,G. Cao,Chujie Chen,U. Chowdhury,Karl J. Clark,J. I. Collar,P. S. Cooper,M. B. Crisler,G. Crowder,C. E. Dahl,Mala Das,S. Fallows,J. Farine,Ivan Felis,R. Filgas,F. Girard,G. Giroux,J. Hall,O. Harris,Eric W. Hoppe,M. Jin,C. B. Krauss,M. Laurin,I. Lawson,A. Leblanc,Ilan Levine,W. H. Lippincott,F. Mamedov,Deepam Maurya,P. Mitra,T. Nania,R. Neilson,A. J. Noble,S. Olson,Amber M. Ortega,A. Plante,R. Podviyanuk,Shashank Priya,A. E. Robinson,A. Roeder,R. Rucinski,O. Scallon,Satyajit Seth,A. Sonnenschein,N. Starinski,I. Stekl,F. Tardif,E. Vázquez-Jáuregui,J. Wells,U. Wichoski,Yongke Yan,V. Zacek,Jie Zhang +61 more
TL;DR: These results set the most stringent direct-detection constraint to date on the weakly interacting massive particle (WIMP)-proton spin-dependent cross section at 3.4×10^{-41} cm^{2} for a 30-GeV c^{-2} WIMP, more than 1 order of magnitude improvement from previous PICO results.