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; L. Baudis; D. A. Bauer; J. Beaty; P. L. Brink; T. Bruch; R. Bunker; S. Burke; B. Cabrera; D. O. Caldwell; J. Cooley; P. Cushman; F. DeJongh; M. R. Dragowsky; L. Duong; J. Emes; E. Figueroa-Feliciano; J. Filippini; M. Fritts; R. J. Gaitskell; S. R. Golwala; D. R. Grant; J. Hall; R. Hennings-Yeomans; S. Hertel; D. Holmgren; M. E. Huber; R. Mahapatra; V. Mandic; K. A. McCarthy; N. Mirabolfathi; H. Nelson; L. Novak; R. W. Ogburn; M. Pyle; X. Qiu; E. Ramberg; W. Rau; A. Reisetter; T. Saab; B. Sadoulet; J. Sander; R. Schmitt; R. W. Schnee; D. N. Seitz; B. Serfass; A. Sirois; K. M. Sundqvist; M. Tarka; A. Tomada; G. Wang; S. Yellin; J. Yoo; B. A. Young

doi:10.1103/PhysRevLett.102.011301

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, L. Baudis, D. A. Bauer, J. Beaty, P. L. Brink, T. Bruch, R. Bunker, S. Burke, B. Cabrera, D. O. Caldwell, J. Cooley, P. Cushman, F. DeJongh, M. R. Dragowsky, L. Duong, J. EmesE. Figueroa-Feliciano, J. Filippini, M. Fritts, R. J. Gaitskell, S. R. Golwala, D. R. Grant, J. Hall, R. Hennings-Yeomans, S. Hertel, D. Holmgren, M. E. Huber, R. Mahapatra, V. Mandic, K. A. McCarthy, N. Mirabolfathi, H. Nelson, L. Novak, R. W. Ogburn, M. Pyle, X. Qiu, E. Ramberg, W. Rau, A. Reisetter, T. Saab, B. Sadoulet, J. Sander, R. Schmitt, R. W. Schnee, D. N. Seitz, B. Serfass, A. Sirois, K. M. Sundqvist, M. Tarka, A. Tomada, G. Wang, S. Yellin, J. Yoo, B. A. Young

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Abstract

We report results from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory (CDMS II) featuring the full complement of 30 detectors. 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 6.6×10-44cm2 (4.6×10-44cm2 when combined with previous CDMS II data) at the 90% confidence level for a WIMP mass of 60GeV/c2. This achieves the best sensitivity for dark matter WIMPs with masses above 44GeV/c2, and significantly restricts the parameter space for some favored supersymmetric models.

Original language	English (US)
Article number	011301
Journal	Physical review letters
Volume	102
Issue number	1
DOIs	https://doi.org/10.1103/PhysRevLett.102.011301
State	Published - Jan 5 2009
Externally published	Yes

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General Physics and Astronomy

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10.1103/PhysRevLett.102.011301

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Ahmed, Z., Akerib, D. S., Arrenberg, S., Attisha, M. J., Bailey, C. N., Baudis, L., Bauer, D. A., Beaty, J., Brink, P. L., Bruch, T., Bunker, R., Burke, S., Cabrera, B., Caldwell, D. O., Cooley, J., Cushman, P., DeJongh, F., Dragowsky, M. R., Duong, L., ... Young, B. A. (2009). Search for weakly interacting massive particles with the first five-tower data from the cryogenic dark matter search at the Soudan Underground Laboratory. Physical review letters, 102(1), Article 011301. https://doi.org/10.1103/PhysRevLett.102.011301

Ahmed, Z, Akerib, DS, Arrenberg, S, Attisha, MJ, Bailey, CN, Baudis, L, Bauer, DA, Beaty, J, Brink, PL, Bruch, T, Bunker, R, Burke, S, Cabrera, B, Caldwell, DO, Cooley, J, Cushman, P, DeJongh, F, Dragowsky, MR, Duong, L, Emes, J, Figueroa-Feliciano, E, Filippini, J, Fritts, M, Gaitskell, RJ, Golwala, SR, Grant, DR, Hall, J, Hennings-Yeomans, R, Hertel, S, Holmgren, D, Huber, ME, Mahapatra, R, Mandic, V, McCarthy, KA, Mirabolfathi, N, Nelson, H, Novak, L, Ogburn, RW, Pyle, M, Qiu, X, Ramberg, E, Rau, W, Reisetter, A, Saab, T, Sadoulet, B, Sander, J, Schmitt, R, Schnee, RW, Seitz, DN, Serfass, B, Sirois, A, Sundqvist, KM, Tarka, M, Tomada, A, Wang, G, Yellin, S, Yoo, J & Young, BA 2009, 'Search for weakly interacting massive particles with the first five-tower data from the cryogenic dark matter search at the Soudan Underground Laboratory', Physical review letters, vol. 102, no. 1, 011301. https://doi.org/10.1103/PhysRevLett.102.011301

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title = "Search for weakly interacting massive particles with the first five-tower data from the cryogenic dark matter search at the Soudan Underground Laboratory",

abstract = "We report results from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory (CDMS II) featuring the full complement of 30 detectors. 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 6.6×10-44cm2 (4.6×10-44cm2 when combined with previous CDMS II data) at the 90% confidence level for a WIMP mass of 60GeV/c2. This achieves the best sensitivity for dark matter WIMPs with masses above 44GeV/c2, and significantly restricts the parameter space for some favored supersymmetric models.",

author = "Z. Ahmed and Akerib, {D. S.} and S. Arrenberg and Attisha, {M. J.} and Bailey, {C. N.} and L. Baudis and Bauer, {D. A.} and J. Beaty and Brink, {P. L.} and T. Bruch and R. Bunker and S. Burke and B. Cabrera and Caldwell, {D. O.} and J. Cooley and P. Cushman and F. DeJongh and Dragowsky, {M. R.} and L. Duong and J. Emes and E. Figueroa-Feliciano and J. Filippini and M. Fritts and Gaitskell, {R. J.} and Golwala, {S. R.} and Grant, {D. R.} and J. Hall and R. Hennings-Yeomans and S. Hertel and D. Holmgren and Huber, {M. E.} and R. Mahapatra and V. Mandic and McCarthy, {K. A.} and N. Mirabolfathi and H. Nelson and L. Novak and Ogburn, {R. W.} and M. Pyle and X. Qiu and E. Ramberg and W. Rau and A. Reisetter and T. Saab and B. Sadoulet and J. Sander and R. Schmitt and Schnee, {R. W.} and Seitz, {D. N.} and B. Serfass and A. Sirois and Sundqvist, {K. M.} and M. Tarka and A. Tomada and G. Wang and S. Yellin and J. Yoo and Young, {B. A.}",

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doi = "10.1103/PhysRevLett.102.011301",

language = "English (US)",

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T1 - Search for weakly interacting massive particles with the first five-tower data from the cryogenic dark matter search at the Soudan Underground Laboratory

AU - Ahmed, Z.

AU - Akerib, D. S.

AU - Arrenberg, S.

AU - Attisha, M. J.

AU - Bailey, C. N.

AU - Baudis, L.

AU - Bauer, D. A.

AU - Beaty, J.

AU - Brink, P. L.

AU - Bruch, T.

AU - Bunker, R.

AU - Burke, S.

AU - Cabrera, B.

AU - Caldwell, D. O.

AU - Cooley, J.

AU - Cushman, P.

AU - DeJongh, F.

AU - Dragowsky, M. R.

AU - Duong, L.

AU - Emes, J.

AU - Figueroa-Feliciano, E.

AU - Filippini, J.

AU - Fritts, M.

AU - Gaitskell, R. J.

AU - Golwala, S. R.

AU - Grant, D. R.

AU - Hall, J.

AU - Hennings-Yeomans, R.

AU - Hertel, S.

AU - Holmgren, D.

AU - Huber, M. E.

AU - Mahapatra, R.

AU - Mandic, V.

AU - McCarthy, K. A.

AU - Mirabolfathi, N.

AU - Nelson, H.

AU - Novak, L.

AU - Ogburn, R. W.

AU - Pyle, M.

AU - Qiu, X.

AU - Ramberg, E.

AU - Rau, W.

AU - Reisetter, A.

AU - Saab, T.

AU - Sadoulet, B.

AU - Sander, J.

AU - Schmitt, R.

AU - Schnee, R. W.

AU - Seitz, D. N.

AU - Serfass, B.

AU - Sirois, A.

AU - Sundqvist, K. M.

AU - Tarka, M.

AU - Tomada, A.

AU - Wang, G.

AU - Yellin, S.

AU - Yoo, J.

AU - Young, B. A.

PY - 2009/1/5

Y1 - 2009/1/5

N2 - We report results from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory (CDMS II) featuring the full complement of 30 detectors. 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 6.6×10-44cm2 (4.6×10-44cm2 when combined with previous CDMS II data) at the 90% confidence level for a WIMP mass of 60GeV/c2. This achieves the best sensitivity for dark matter WIMPs with masses above 44GeV/c2, and significantly restricts the parameter space for some favored supersymmetric models.

AB - We report results from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory (CDMS II) featuring the full complement of 30 detectors. 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 6.6×10-44cm2 (4.6×10-44cm2 when combined with previous CDMS II data) at the 90% confidence level for a WIMP mass of 60GeV/c2. This achieves the best sensitivity for dark matter WIMPs with masses above 44GeV/c2, and significantly restricts the parameter space for some favored supersymmetric models.

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U2 - 10.1103/PhysRevLett.102.011301

DO - 10.1103/PhysRevLett.102.011301

M3 - Article

AN - SCOPUS:58649118638

SN - 0031-9007

VL - 102

JO - Physical review letters

JF - Physical review letters

IS - 1

M1 - 011301

ER -

Search for weakly interacting massive particles with the first five-tower data from the cryogenic dark matter search at the Soudan Underground Laboratory

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