David O. Caldwell
University of California, Santa Barbara
134 Papers
973 Citations
David O. Caldwell is an academic researcher from University of California, Santa Barbara. The author has contributed to research in topics: Dark matter & Neutrino. The author has an hindex of 34, co-authored 134 publications. Previous affiliations of David O. Caldwell include University of California, Berkeley & University of California.
Chat about Author
Papers
Dark matter search results from the CDMS II experiment.
Jodi Cooley,Z. Ahmed,D. S. Akerib,S. Arrenberg,C. N. Bailey,D. Balakishiyeva,Laura Baudis,D. A. Bauer,P. L. Brink,T. Bruch,R. Bunker,Blas Cabrera,David O. Caldwell,P. Cushman,Miguel Daal,F. DeJongh,M. R. Dragowsky,L. Duong,S. Fallows,Enectali Figueroa-Feliciano,Jeffrey P. Filippini,Matthew Fritts,Sunil Golwala,Darren Grant,J. Hall,R. Hennings-Yeomans,S. A. Hertel,Donald J. Holmgren,L. Hsu,Martin E. Huber,O. Kamaev,M. Kiveni,M. Kos,Steven W. Leman,R. Mahapatra,Vuk Mandic,Kevin A. McCarthy,N. Mirabolfathi,David Moore,H. N. Nelson,R. W. Ogburn,A. Phipps,M. Pyle,X. Oiu,E. J. Ramberg,W. Rau,A. Resetter,A. Resetter,Tarek Saab,Bernard Sadoulet,Bernard Sadoulet,J. Sander,R. W. Schnee,D. N. Seitz,B. Serfass,K. M. Sundqvist,M. Tarka,P. Wikus,S. J. Yellin,S. J. Yellin,J. Yoo,Betty A. Young,Jie Zhang +62 more
TL;DR: The results from the completed Cryogenic Dark Matter Search (CDMS II) experiment, which searched for dark matter in the form of weakly interacting massive particles (WIMP), cannot be interpreted with confidence as evidence for WIMP interactions, but neither event can be ruled out as representing signal.
Search for low-mass weakly interacting massive particles with SuperCDMS.
R. Agnese,Adam Anderson,M. Asai,D. Balakishiyeva,R. Basu Thakur,D. A. Bauer,J. Beaty,J. Billard,A. W. Borgland,M. A. Bowles,D. Brandt,P. L. Brink,R. Bunker,Blas Cabrera,David O. Caldwell,David G. Cerdeño,H. Chagani,Yan Chen,M. Cherry,Jodi Cooley,B. Cornell,C. H. Crewdson,P. Cushman,Miguel Daal,D. Devaney,P. Di Stefano,E. Do Couto E Silva,T. Doughty,L. Esteban,S. Fallows,Enectali Figueroa-Feliciano,G. Godfrey,Sunil Golwala,J. Hall,Sissel Hansen,H. R. Harris,S. A. Hertel,B. A. Hines,T. Hofer,Donald J. Holmgren,L. Hsu,Martin E. Huber,A. Jastram,O. Kamaev,B. Kara,M. H. Kelsey,S. Kenany,A. Kennedy,M. Kiveni,K. Koch,A. Leder,B. Loer,E. Lopez Asamar,R. Mahapatra,Vuk Mandic,Cristián Martínez,Kevin A. McCarthy,N. Mirabolfathi,Robert A. Moffatt,R. H. Nelson,L. Novak,K. L. Page,R. Partridge,M. Pepin,A. Phipps,M. Platt,K. Prasad,Matt Pyle,H. Qiu,W. Rau,P. Redl,A. Reisetter,R. Resch,Y. Ricci,M. Ruschman,Tarek Saab,Bernard Sadoulet,J. Sander,R. Schmitt,K. Schneck,R. W. Schnee,S. Scorza,D. N. Seitz,B. Serfass,B. Shank,Danielle Speller,Astrid Tomada,S. Upadhyayula,A. N. Villano,B. Welliver,Douglas Wright,S. J. Yellin,J. J. Yen,Betty A. Young,J. Zhang +94 more
TL;DR: The first search for weakly interacting massive particles (WIMPs) using the background rejection capabilities of SuperCDMS was reported in this article, where an exposure of 577 kg days was analyzed for WIMPs with mass <30 ǫ, with the signal region blinded.
New Results from the Search for Low-Mass Weakly Interacting Massive Particles with the CDMS Low Ionization Threshold Experiment
R. Agnese,Adam Anderson,Tsuguo Aramaki,M. Asai,W. Baker,D. Balakishiyeva,D. Barker,R. Basu Thakur,D. A. Bauer,J. Billard,A. Borgland,M. A. Bowles,P. L. Brink,R. Bunker,Blas Cabrera,David O. Caldwell,R. Calkins,David G. Cerdeño,H. Chagani,Yi Chen,Jodi Cooley,B. Cornell,P. Cushman,Miguel Daal,P. Di Stefano,T. Doughty,L. Esteban,S. Fallows,Enectali Figueroa-Feliciano,M. Ghaith,G. L. Godfrey,Sunil Golwala,J. Hall,H. R. Harris,T. Hofer,Donald J. Holmgren,L. Hsu,Martin E. Huber,D. Jardin,A. Jastram,O. Kamaev,B. Kara,M. H. Kelsey,A. Kennedy,A. Leder,B. Loer,E. Lopez Asamar,P. Lukens,R. Mahapatra,Vuk Mandic,N. Mast,N. Mirabolfathi,Robert A. Moffatt,J. D. Morales Mendoza,S. M. Oser,K. L. Page,W. A. Page,R. Partridge,M. Pepin,A. Phipps,K. Prasad,Matt Pyle,H. Qiu,W. Rau,P. Redl,A. Reisetter,Y. Ricci,Amy Roberts,H. E. Rogers,Tarek Saab,Bernard Sadoulet,J. Sander,K. Schneck,R. W. Schnee,S. Scorza,B. Serfass,B. Shank,Danielle Speller,D. Toback,R. Underwood,S. Upadhyayula,A. N. Villano,B. Welliver,John Wilson,D. H. Wright,S. J. Yellin,J. J. Yen,Betty A. Young,J. Zhang +88 more
TL;DR: The CDMS low ionization threshold experiment (CDMSlite) uses cryogenic germanium detectors operated at a relatively high bias voltage to amplify the phonon signal in the search for weakly interacting massive particles (WIMPs).
Search for weakly interacting massive particles with the first five-tower data from the cryogenic dark matter search at the soudan underground laboratory.
Z. Ahmed,D. S. Akerib,S. Arrenberg,M. J. Attisha,C. N. Bailey,Laura Baudis,D. A. Bauer,J. Beaty,P. L. Brink,T. Bruch,R. Bunker,S. Burke,Blas Cabrera,David O. Caldwell,Jodi Cooley,P. Cushman,F. DeJongh,M. R. Dragowsky,L. Duong,J. Emes,Enectali Figueroa-Feliciano,Jeffrey P. Filippini,Matthew Fritts,R. J. Gaitskell,Sunil Golwala,Darren Grant,J. Hall,R. Hennings-Yeomans,S. A. Hertel,Donald J. Holmgren,Martin E. Huber,R. Mahapatra,Vuk Mandic,Kevin A. McCarthy,N. Mirabolfathi,H. N. Nelson,L. Novak,R. W. Ogburn,M. Pyle,X. Qiu,E. J. Ramberg,W. Rau,A. Reisetter,Tarek Saab,Bernard Sadoulet,Bernard Sadoulet,J. Sander,R. Schmitt,R. W. Schnee,D. N. Seitz,B. Serfass,Adam Sirois,K. M. Sundqvist,M. Tarka,Astrid Tomada,G. Wang,S. J. Yellin,S. J. Yellin,J. Yoo,Betty A. Young +59 more
TL;DR: In this article, the authors report results from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory (CDMS II) featuring the full complement of 30 detectors, and a blind analysis of data taken between October 2006 and July 2007 sets an upper limit on the weakly interacting massive particle (WIMP) nucleon spin-independent cross section of 6.6 x 10^(-44) cm^2.
529
•Posted Content
Silicon Detector Dark Matter Results from the Final Exposure of CDMS II
R. Agnese,Z. Ahmed,Adam Anderson,S. Arrenberg,D. Balakishiyeva,R. Basu Thakur,D. A. Bauer,J. Billard,A. W. Borgland,D. Brandt,P. L. Brink,T. Bruch,R. Bunker,Blas Cabrera,David O. Caldwell,David G. Cerdeño,H. Chagani,Jodi Cooley,B. Cornell,C. H. Crewdson,P. Cushman,Miguel Daal,F. DeJongh,E. Do Couto E Silva,T. Doughty,L. Esteban,S. Fallows,Enectali Figueroa-Feliciano,Jeffrey P. Filippini,John Fox,Matthew Fritts,G.L. Godfrey,Sunil Golwala,J. Hall,R. H. Harris,S. A. Hertel,T. Hofer,Donald J. Holmgren,L. Hsu,Martin E. Huber,A. Jastram,O. Kamaev,B. Kara,M. H. Kelsey,A. Kennedy,Peter S. Kim,M. Kiveni,K. Koch,M. Kos,Steven W. Leman,Ben Loer,E. Lopez Asamar,R. Mahapatra,Vuk Mandic,Cristián Martínez,Kevin A. McCarthy,N. Mirabolfathi,Robert A. Moffatt,David Moore,P. Nadeau,R. H. Nelson,K. L. Page,R. Partridge,M. Pepin,A. Phipps,K. Prasad,M. Pyle,H. Qiu,W. Rau,P. Redl,A. Reisetter,Y. Ricci,Tarek Saab,Bernard Sadoulet,J. Sander,K. Schneck,R. W. Schnee,S. Scorza,B. Serfass,B. Shank,Danielle Speller,K. M. Sundqvist,A. N. Villano,B. Welliver,D. H. Wright,S. J. Yellin,J. J. Yen,J. Yoo,Betty A. Young,J. Zhang +89 more
TL;DR: Results of a search for weakly interacting massive particles (WIMPS) with the silicon detectors of the CDMS II experiment revealed three WIMP-candidate events with a surface-event background estimate of 0.41, with a profile likelihood ratio test giving a 0.19% probability for the known-background-only hypothesis when tested against the alternative WIMp+background hypothesis.
428