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9 results on '"T. Doughty"'

1. Silicon detector dark matter results from the final exposure of CDMS II

Author

Matthew Fritts, Jeffrey P. Filippini, G.L. Godfrey, Jodi Cooley, M. H. Kelsey, Vuk Mandic, K. Prasad, S. A. Hertel, P. L. Brink, David O. Caldwell, Y. Ricci, T. Hofer, P. Nadeau, Steven W. Leman, M. Kos, B. Shank, D. Balakishiyeva, Martin E. Huber, Donald J. Holmgren, P. Cushman, J. Sander, K. Koch, A. W. Borgland, C. H. Crewdson, D. A. Bauer, L. Esteban, Miguel Daal, R. Basu Thakur, R. Partridge, A. Jastram, K. L. Page, S. Scorza, P. Redl, B. Loer, J. Hall, B. Serfass, R. H. Harris, Cristián Martínez, David Moore, Robert A. Moffatt, Bernard Sadoulet, S. Arrenberg, P. Kim, K. Schneck, J. J. Yen, H. Qiu, B. Kara, Z. Ahmed, R. Bunker, A. N. Villano, T. Bruch, B. Welliver, Betty A. Young, Sunil Golwala, A. Kennedy, Danielle Speller, David G. Cerdeño, N. Mirabolfathi, Douglas Wright, A. Reisetter, B. Cornell, Blas Cabrera, A. Phipps, K. M. Sundqvist, L. Hsu, W. Rau, R. Mahapatra, Kevin A. McCarthy, H. Chagani, R. W. Schnee, J. Fox, O. Kamaev, J. Zhang, F. DeJongh, E. Do Couto E Silva, Adam Anderson, D. Brandt, R. Agnese, S. Fallows, Enectali Figueroa-Feliciano, M. Kiveni, S. J. Yellin, Matt Pyle, E. Lopez Asamar, Tarek Saab, J. Yoo, J. Billard, M. Pepin, R. H. Nelson, T. Doughty, and UAM. Departamento de Física Teórica

Subjects
Particle physics, Physics - Instrumentation and Detectors, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Dark matter, FOS: Physical sciences, General Physics and Astronomy, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Recoil, WIMP, 0103 physical sciences, Neutron, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, 010308 nuclear & particles physics, Física, Instrumentation and Detectors (physics.ins-det), Confidence interval, Semiconductor detector, Likelihood-ratio test, Weakly interacting massive particles, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We report results of a search for Weakly Interacting Massive Particles (WIMPS) with the silicon detectors of the CDMS II experiment. This blind analysis of 140.2 kg-days of data taken between July 2007 and September 2008 revealed three WIMP-candidate events with a surface-event background estimate of 0.41^{+0.20}_{-0.08}(stat.)^{+0.28}_{-0.24}(syst.). Other known backgrounds from neutrons and 206Pb are limited to < 0.13 and, 5 pages, 4 figures, as accepted by PRL

Published
2013

2. Erratum: First Dark Matter Constraints from a SuperCDMS Single-Charge Sensitive Detector [Phys. Rev. Lett. 121, 051301 (2018)].

Author

Agnese R, Aralis T, Aramaki T, Arnquist IJ, Azadbakht E, Baker W, Banik S, Barker D, Bauer DA, Binder T, Bowles MA, Brink PL, Bunker R, Cabrera B, Calkins R, Cartaro C, Cerdeño DG, Chang YY, Cooley J, Cornell B, Cushman P, Di Stefano PCF, Doughty T, Fascione E, Figueroa-Feliciano E, Fink C, Fritts M, Gerbier G, Germond R, Ghaith M, Golwala SR, Harris HR, Hong Z, Hoppe EW, Hsu L, Huber ME, Iyer V, Jardin D, Jena C, Kelsey MH, Kennedy A, Kubik A, Kurinsky NA, Lawrence RE, Leyva JV, Loer B, Lopez Asamar E, Lukens P, MacDonell D, Mahapatra R, Mandic V, Mast N, Miller EH, Mirabolfathi N, Mohanty B, Morales Mendoza JD, Nelson J, Orrell JL, Oser SM, Page WA, Partridge R, Pepin M, Phipps A, Ponce F, Poudel S, Pyle M, Qiu H, Rau W, Reisetter A, Reynolds T, Roberts A, Robinson AE, Rogers HE, Romani RK, Saab T, Sadoulet B, Sander J, Scarff A, Schnee RW, Scorza S, Senapati K, Serfass B, So J, Speller D, Stanford C, Stein M, Street J, Tanaka HA, Toback D, Underwood R, Villano AN, von Krosigk B, Watkins SL, Wilson JS, Wilson MJ, Winchell J, Wright DH, Yellin S, Young BA, Zhang X, and Zhao X

Abstract

This corrects the article DOI: 10.1103/PhysRevLett.121.051301.

Published
2019
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3. First Dark Matter Constraints from a SuperCDMS Single-Charge Sensitive Detector.

Author

Agnese R, Aralis T, Aramaki T, Arnquist IJ, Azadbakht E, Baker W, Banik S, Barker D, Bauer DA, Binder T, Bowles MA, Brink PL, Bunker R, Cabrera B, Calkins R, Cartaro C, Cerdeño DG, Chang YY, Cooley J, Cornell B, Cushman P, Di Stefano PCF, Doughty T, Fascione E, Figueroa-Feliciano E, Fink C, Fritts M, Gerbier G, Germond R, Ghaith M, Golwala SR, Harris HR, Hong Z, Hoppe EW, Hsu L, Huber ME, Iyer V, Jardin D, Jena C, Kelsey MH, Kennedy A, Kubik A, Kurinsky NA, Lawrence RE, Leyva JV, Loer B, Lopez Asamar E, Lukens P, MacDonell D, Mahapatra R, Mandic V, Mast N, Miller EH, Mirabolfathi N, Mohanty B, Morales Mendoza JD, Nelson J, Orrell JL, Oser SM, Page WA, Partridge R, Pepin M, Phipps A, Ponce F, Poudel S, Pyle M, Qiu H, Rau W, Reisetter A, Reynolds T, Roberts A, Robinson AE, Rogers HE, Romani RK, Saab T, Sadoulet B, Sander J, Scarff A, Schnee RW, Scorza S, Senapati K, Serfass B, So J, Speller D, Stanford C, Stein M, Street J, Tanaka HA, Toback D, Underwood R, Villano AN, von Krosigk B, Watkins SL, Wilson JS, Wilson MJ, Winchell J, Wright DH, Yellin S, Young BA, Zhang X, and Zhao X

Abstract

We present the first limits on inelastic electron-scattering dark matter and dark photon absorption using a prototype SuperCDMS detector having a charge resolution of 0.1 electron-hole pairs (CDMS HVeV, a 0.93 g CDMS high-voltage device). These electron-recoil limits significantly improve experimental constraints on dark matter particles with masses as low as 1  MeV/c^{2}. We demonstrate a sensitivity to dark photons competitive with other leading approaches but using substantially less exposure (0.49 g d). These results demonstrate the scientific potential of phonon-mediated semiconductor detectors that are sensitive to single electronic excitations.

Published
2018
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4. Results from the Super Cryogenic Dark Matter Search Experiment at Soudan.

Author

Agnese R, Aramaki T, Arnquist IJ, Baker W, Balakishiyeva D, Banik S, Barker D, Basu Thakur R, Bauer DA, Binder T, Bowles MA, Brink PL, Bunker R, Cabrera B, Caldwell DO, Calkins R, Cartaro C, Cerdeño DG, Chang Y, Chen Y, Cooley J, Cornell B, Cushman P, Daal M, Di Stefano PCF, Doughty T, Fascione E, Figueroa-Feliciano E, Fritts M, Gerbier G, Germond R, Ghaith M, Godfrey GL, Golwala SR, Hall J, Harris HR, Hong Z, Hoppe EW, Hsu L, Huber ME, Iyer V, Jardin D, Jastram A, Jena C, Kelsey MH, Kennedy A, Kubik A, Kurinsky NA, Loer B, Lopez Asamar E, Lukens P, MacDonell D, Mahapatra R, Mandic V, Mast N, Miller EH, Mirabolfathi N, Mohanty B, Morales Mendoza JD, Nelson J, Orrell JL, Oser SM, Page K, Page WA, Partridge R, Penalver Martinez M, Pepin M, Phipps A, Poudel S, Pyle M, Qiu H, Rau W, Redl P, Reisetter A, Reynolds T, Roberts A, Robinson AE, Rogers HE, Saab T, Sadoulet B, Sander J, Schneck K, Schnee RW, Scorza S, Senapati K, Serfass B, Speller D, Stein M, Street J, Tanaka HA, Toback D, Underwood R, Villano AN, von Krosigk B, Welliver B, Wilson JS, Wilson MJ, Wright DH, Yellin S, Yen JJ, Young BA, Zhang X, and Zhao X

Abstract

We report the result of a blinded search for weakly interacting massive particles (WIMPs) using the majority of the SuperCDMS Soudan data set. With an exposure of 1690 kg d, a single candidate event is observed, consistent with expected backgrounds. This analysis (combined with previous Ge results) sets an upper limit on the spin-independent WIMP-nucleon cross section of 1.4×10^{-44} (1.0×10^{-44})  cm^{2} at 46  GeV/c^{2}. These results set the strongest limits for WIMP-germanium-nucleus interactions for masses >12  GeV/c^{2}.

Published
2018
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5. New Results from the Search for Low-Mass Weakly Interacting Massive Particles with the CDMS Low Ionization Threshold Experiment.

Author

Agnese R, Anderson AJ, Aramaki T, Asai M, Baker W, Balakishiyeva D, Barker D, Basu Thakur R, Bauer DA, Billard J, Borgland A, Bowles MA, Brink PL, Bunker R, Cabrera B, Caldwell DO, Calkins R, Cerdeno DG, Chagani H, Chen Y, Cooley J, Cornell B, Cushman P, Daal M, Di Stefano PC, Doughty T, Esteban L, Fallows S, Figueroa-Feliciano E, Ghaith M, Godfrey GL, Golwala SR, Hall J, Harris HR, Hofer T, Holmgren D, Hsu L, Huber ME, Jardin D, Jastram A, Kamaev O, Kara B, Kelsey MH, Kennedy A, Leder A, Loer B, Lopez Asamar E, Lukens P, Mahapatra R, Mandic V, Mast N, Mirabolfathi N, Moffatt RA, Morales Mendoza JD, Oser SM, Page K, Page WA, Partridge R, Pepin M, Phipps A, Prasad K, Pyle M, Qiu H, Rau W, Redl P, Reisetter A, Ricci Y, Roberts A, Rogers HE, Saab T, Sadoulet B, Sander J, Schneck K, Schnee RW, Scorza S, Serfass B, Shank B, Speller D, Toback D, Underwood R, Upadhyayula S, Villano AN, Welliver B, Wilson JS, Wright DH, Yellin S, Yen JJ, Young BA, and Zhang J

Abstract

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). Results are presented from the second CDMSlite run with an exposure of 70 kg day, which reached an energy threshold for electron recoils as low as 56 eV. A fiducialization cut reduces backgrounds below those previously reported by CDMSlite. New parameter space for the WIMP-nucleon spin-independent cross section is excluded for WIMP masses between 1.6 and 5.5  GeV/c^{2}.

Published
2016
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6. First direct limits on lightly ionizing particles with electric charge less than e/6.

Author

Agnese R, Anderson AJ, Balakishiyeva D, Basu Thakur R, Bauer DA, Billard J, Borgland A, Bowles MA, Brandt D, Brink PL, Bunker R, Cabrera B, Caldwell DO, Cerdeno DG, Chagani H, Chen Y, Cooley J, Cornell B, Crewdson CH, Cushman P, Daal M, Di Stefano PC, Doughty T, Esteban L, Fallows S, Figueroa-Feliciano E, Godfrey GL, Golwala SR, Hall J, Harris HR, Hertel SA, Hofer T, Holmgren D, Hsu L, Huber ME, Jastram A, Kamaev O, Kara B, Kelsey MH, Kennedy A, Kiveni M, Koch K, Leder A, Loer B, Lopez Asamar E, Mahapatra R, Mandic V, Martinez C, McCarthy KA, Mirabolfathi N, Moffatt RA, Moore DC, Nelson H, Nelson RH, Ogburn RW, Page K, Page WA, Partridge R, Pepin M, Phipps A, Prasad K, Pyle M, Qiu H, Rau W, Redl P, Reisetter A, Ricci Y, Rogers HE, Saab T, Sadoulet B, Sander J, Schneck K, Schnee RW, Scorza S, Serfass B, Shank B, Speller D, Upadhyayula S, Villano AN, Welliver B, Wright DH, Yellin S, Yen JJ, Young BA, and Zhang J

Abstract

While the standard model of particle physics does not include free particles with fractional charge, experimental searches have not ruled out their existence. We report results from the Cryogenic Dark Matter Search (CDMS II) experiment that give the first direct-detection limits for cosmogenically produced relativistic particles with electric charge lower than e/6. A search for tracks in the six stacked detectors of each of two of the CDMS II towers finds no candidates, thereby excluding new parameter space for particles with electric charges between e/6 and e/200.

Published
2015
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7. Search for low-mass weakly interacting massive particles with SuperCDMS.

Author

Agnese R, Anderson AJ, Asai M, Balakishiyeva D, Basu Thakur R, Bauer DA, Beaty J, Billard J, Borgland A, Bowles MA, Brandt D, Brink PL, Bunker R, Cabrera B, Caldwell DO, Cerdeno DG, Chagani H, Chen Y, Cherry M, Cooley J, Cornell B, Crewdson CH, Cushman P, Daal M, DeVaney D, Di Stefano PC, Silva Edo C, Doughty T, Esteban L, Fallows S, Figueroa-Feliciano E, Godfrey GL, Golwala SR, Hall J, Hansen S, Harris HR, Hertel SA, Hines BA, Hofer T, Holmgren D, Hsu L, Huber ME, Jastram A, Kamaev O, Kara B, Kelsey MH, Kenany S, Kennedy A, Kiveni M, Koch K, Leder A, Loer B, Lopez Asamar E, Mahapatra R, Mandic V, Martinez C, McCarthy KA, Mirabolfathi N, Moffatt RA, Nelson RH, Novak L, Page K, Partridge R, Pepin M, Phipps A, Platt M, Prasad K, Pyle M, Qiu H, Rau W, Redl P, Reisetter A, Resch RW, Ricci Y, Ruschman M, Saab T, Sadoulet B, Sander J, Schmitt RL, Schneck K, Schnee RW, Scorza S, Seitz DN, Serfass B, Shank B, Speller D, Tomada A, Upadhyayula S, Villano AN, Welliver B, Wright DH, Yellin S, Yen JJ, Young BA, and Zhang J

Abstract

We report a first search for weakly interacting massive particles (WIMPs) using the background rejection capabilities of SuperCDMS. An exposure of 577 kg days was analyzed for WIMPs with mass <30  GeV/c(2), with the signal region blinded. Eleven events were observed after unblinding. We set an upper limit on the spin-independent WIMP-nucleon cross section of 1.2×10(-42)  cm(2) at 8  GeV/c(2). This result is in tension with WIMP interpretations of recent experiments and probes new parameter space for WIMP-nucleon scattering for WIMP masses <6  GeV/c(2).

Published
2014
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8. Search for low-mass weakly interacting massive particles using voltage-assisted calorimetric ionization detection in the SuperCDMS experiment.

Author

Agnese R, Anderson AJ, Asai M, Balakishiyeva D, Basu Thakur R, Bauer DA, Billard J, Borgland A, Bowles MA, Brandt D, Brink PL, Bunker R, Cabrera B, Caldwell DO, Cerdeno DG, Chagani H, Cooley J, Cornell B, Crewdson CH, Cushman P, Daal M, Di Stefano PC, Doughty T, Esteban L, Fallows S, Figueroa-Feliciano E, Godfrey GL, Golwala SR, Hall J, Harris HR, Hertel SA, Hofer T, Holmgren D, Hsu L, Huber ME, Jastram A, Kamaev O, Kara B, Kelsey MH, Kennedy A, Kiveni M, Koch K, Loer B, Lopez Asamar E, Mahapatra R, Mandic V, Martinez C, McCarthy KA, Mirabolfathi N, Moffatt RA, Moore DC, Nadeau P, Nelson RH, Page K, Partridge R, Pepin M, Phipps A, Prasad K, Pyle M, Qiu H, Rau W, Redl P, Reisetter A, Ricci Y, Saab T, Sadoulet B, Sander J, Schneck K, Schnee RW, Scorza S, Serfass B, Shank B, Speller D, Villano AN, Welliver B, Wright DH, Yellin S, Yen JJ, Young BA, and Zhang J

Abstract

SuperCDMS is an experiment designed to directly detect weakly interacting massive particles (WIMPs), a favored candidate for dark matter ubiquitous in the Universe. In this Letter, we present WIMP-search results using a calorimetric technique we call CDMSlite, which relies on voltage-assisted Luke-Neganov amplification of the ionization energy deposited by particle interactions. The data were collected with a single 0.6 kg germanium detector running for ten live days at the Soudan Underground Laboratory. A low energy threshold of 170  eVee (electron equivalent) was obtained, which allows us to constrain new WIMP-nucleon spin-independent parameter space for WIMP masses below 6  GeV/c2.

Published
2014
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9. Silicon detector dark matter results from the final exposure of CDMS II.

Author

Agnese R, Ahmed Z, Anderson AJ, Arrenberg S, Balakishiyeva D, Basu Thakur R, Bauer DA, Billard J, Borgland A, Brandt D, Brink PL, Bruch T, Bunker R, Cabrera B, Caldwell DO, Cerdeno DG, Chagani H, Cooley J, Cornell B, Crewdson CH, Cushman P, Daal M, Dejongh F, do Couto e Silva E, Doughty T, Esteban L, Fallows S, Figueroa-Feliciano E, Filippini J, Fox J, Fritts M, Godfrey GL, Golwala SR, Hall J, Harris RH, Hertel SA, Hofer T, Holmgren D, Hsu L, Huber ME, Jastram A, Kamaev O, Kara B, Kelsey MH, Kennedy A, Kim P, Kiveni M, Koch K, Kos M, Leman SW, Loer B, Lopez Asamar E, Mahapatra R, Mandic V, Martinez C, McCarthy KA, Mirabolfathi N, Moffatt RA, Moore DC, Nadeau P, Nelson RH, Page K, Partridge R, Pepin M, Phipps A, Prasad K, Pyle M, Qiu H, Rau W, Redl P, Reisetter A, Ricci Y, Saab T, Sadoulet B, Sander J, Schneck K, Schnee RW, Scorza S, Serfass B, Shank B, Speller D, Sundqvist KM, Villano AN, Welliver B, Wright DH, Yellin S, Yen JJ, Yoo J, Young BA, and Zhang J

Abstract

We report results of a search for weakly interacting massive particles (WIMPS) with the silicon detectors of the CDMS II experiment. This blind analysis of 140.2 kg day of data taken between July 2007 and September 2008 revealed three WIMP-candidate events with a surface-event background estimate of 0.41(-0.08)(+0.20)(stat)(-0.24)(+0.28)(syst). Other known backgrounds from neutrons and 206Pb are limited to <0.13 and <0.08 events at the 90% confidence level, respectively. The exposure of this analysis is equivalent to 23.4 kg day for a recoil energy range of 7-100 keV for a WIMP of mass 10  GeV/c2. The probability that the known backgrounds would produce three or more events in the signal region is 5.4%. A profile likelihood ratio test of the three events that includes the measured recoil energies gives a 0.19% probability for the known-background-only hypothesis when tested against the alternative WIMP+background hypothesis. The highest likelihood occurs for a WIMP mass of 8.6  GeV/c2 and WIMP-nucleon cross section of 1.9×10(-41)  cm2.

Published
2013
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