First results from the cryogenic dark matter search in the soudan underground laboratory

D. S. Akerib; J. Alvaro-Dean; M. S. Armel-Funkhouser; M. J. Attisha; L. Baudis; D. A. Bauer; J. Beaty; P. L. Brink; R. Bunker; S. P. Burke; B. Cabrera; D. O. Caldwell; D. Callahan; J. P. Castle; C. L. Chang; R. Choate; M. B. Crisler; P. Cushman; R. Dixon; M. R. Dragowsky; D. D. Driscoll; L. Duong; J. Emes; R. Ferril; J. Filippini; R. J. Gaitskell; M. Haldeman; D. Hale; D. Holmgren; M. E. Huber; B. Johnson; W. Johnson; S. Kamat; M. Kozlovsky; L. Kula; S. Kyre; B. Lambin; A. Lu; R. Mahapatra; A. G. Manalaysay; V. Mandic; J. May; R. McDonald; B. Merkel; P. Meunier; N. Mirabolfathi; S. Morrison; H. Nelson; R. Nelson; L. Novak; R. W. Ogburn; S. Orr; T. A. Perera; M. C.Perillo Isaac; E. Ramberg; W. Rau; A. Reisetter; R. R. Ross; T. Saab; B. Sadoulet; J. Sander; C. Savage; R. L. Schmitt; R. W. Schnee; D. N. Seitz; B. Serfass; A. Smith; G. Smith; A. L. Spadafora; K. Sundqvist; J. P.F. Thompson; A. Tomada; G. Wang; J. Williams; S. Yellin; B. A. Young

doi:10.1103/PhysRevLett.93.211301

First results from the cryogenic dark matter search in the soudan underground laboratory

D. S. Akerib, J. Alvaro-Dean, M. S. Armel-Funkhouser, M. J. Attisha, L. Baudis, D. A. Bauer, J. Beaty, P. L. Brink, R. Bunker, S. P. Burke, B. Cabrera, D. O. Caldwell, D. Callahan, J. P. Castle, C. L. Chang, R. Choate, M. B. Crisler, P. Cushman, R. Dixon, M. R. DragowskyD. D. Driscoll, L. Duong, J. Emes, R. Ferril, J. Filippini, R. J. Gaitskell, M. Haldeman, D. Hale, D. Holmgren, M. E. Huber, B. Johnson, W. Johnson, S. Kamat, M. Kozlovsky, L. Kula, S. Kyre, B. Lambin, A. Lu, R. Mahapatra, A. G. Manalaysay, V. Mandic, J. May, R. McDonald, B. Merkel, P. Meunier, N. Mirabolfathi, S. Morrison, H. Nelson, R. Nelson, L. Novak, R. W. Ogburn, S. Orr, T. A. Perera, M. C.Perillo Isaac, E. Ramberg, W. Rau, A. Reisetter, R. R. Ross, T. Saab, B. Sadoulet, J. Sander, C. Savage, R. L. Schmitt, R. W. Schnee, D. N. Seitz, B. Serfass, A. Smith, G. Smith, A. L. Spadafora, K. Sundqvist, J. P.F. Thompson, A. Tomada, G. Wang, J. Williams, S. Yellin, B. A. Young

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Abstract

The first results from the Cryogenic Dark Matter Search for weakly interacting massive particles (WIMP) in the Soudan Underground Laboratory, were investigated. Four Ge and two Si detectors were operated for about 52.6 live days, which provided 19.4 kg d of Ge net exposure after cuts for recoil energies of range between 10 and 100 keV. To define the energy threshold and selection criteria for nuclear-recoil candidates, a blind analysis was performed. These data set the world's lowest exclusion limits on the coherent WIMP-nucleon scalar cross section for all WIMP masses above 15 GeV/c ². The results show that the minimum of this limit at the 90% C.L. is 4×10^-43 cm² at a WIMP mass of 60 GeV/c ².

Original language	English (US)
Article number	211301
Journal	Physical review letters
Volume	93
Issue number	21
DOIs	https://doi.org/10.1103/PhysRevLett.93.211301
State	Published - Nov 19 2004
Externally published	Yes

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General Physics and Astronomy

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Akerib, D. S., Alvaro-Dean, J., Armel-Funkhouser, M. S., Attisha, M. J., Baudis, L., Bauer, D. A., Beaty, J., Brink, P. L., Bunker, R., Burke, S. P., Cabrera, B., Caldwell, D. O., Callahan, D., Castle, J. P., Chang, C. L., Choate, R., Crisler, M. B., Cushman, P., Dixon, R., ... Young, B. A. (2004). First results from the cryogenic dark matter search in the soudan underground laboratory. Physical review letters, 93(21), Article 211301. https://doi.org/10.1103/PhysRevLett.93.211301

Akerib, DS, Alvaro-Dean, J, Armel-Funkhouser, MS, Attisha, MJ, Baudis, L, Bauer, DA, Beaty, J, Brink, PL, Bunker, R, Burke, SP, Cabrera, B, Caldwell, DO, Callahan, D, Castle, JP, Chang, CL, Choate, R, Crisler, MB, Cushman, P, Dixon, R, Dragowsky, MR, Driscoll, DD, Duong, L, Emes, J, Ferril, R, Filippini, J, Gaitskell, RJ, Haldeman, M, Hale, D, Holmgren, D, Huber, ME, Johnson, B, Johnson, W, Kamat, S, Kozlovsky, M, Kula, L, Kyre, S, Lambin, B, Lu, A, Mahapatra, R, Manalaysay, AG, Mandic, V, May, J, McDonald, R, Merkel, B, Meunier, P, Mirabolfathi, N, Morrison, S, Nelson, H, Nelson, R, Novak, L, Ogburn, RW, Orr, S, Perera, TA, Isaac, MCP, Ramberg, E, Rau, W, Reisetter, A, Ross, RR, Saab, T, Sadoulet, B, Sander, J, Savage, C, Schmitt, RL, Schnee, RW, Seitz, DN, Serfass, B, Smith, A, Smith, G, Spadafora, AL, Sundqvist, K, Thompson, JPF, Tomada, A, Wang, G, Williams, J, Yellin, S & Young, BA 2004, 'First results from the cryogenic dark matter search in the soudan underground laboratory', Physical review letters, vol. 93, no. 21, 211301. https://doi.org/10.1103/PhysRevLett.93.211301

@article{dede06bf859040469d1665507f2749c2,

title = "First results from the cryogenic dark matter search in the soudan underground laboratory",

abstract = "The first results from the Cryogenic Dark Matter Search for weakly interacting massive particles (WIMP) in the Soudan Underground Laboratory, were investigated. Four Ge and two Si detectors were operated for about 52.6 live days, which provided 19.4 kg d of Ge net exposure after cuts for recoil energies of range between 10 and 100 keV. To define the energy threshold and selection criteria for nuclear-recoil candidates, a blind analysis was performed. These data set the world's lowest exclusion limits on the coherent WIMP-nucleon scalar cross section for all WIMP masses above 15 GeV/c 2. The results show that the minimum of this limit at the 90% C.L. is 4×10-43 cm2 at a WIMP mass of 60 GeV/c 2.",

author = "Akerib, {D. S.} and J. Alvaro-Dean and Armel-Funkhouser, {M. S.} and Attisha, {M. J.} and L. Baudis and Bauer, {D. A.} and J. Beaty and Brink, {P. L.} and R. Bunker and Burke, {S. P.} and B. Cabrera and Caldwell, {D. O.} and D. Callahan and Castle, {J. P.} and Chang, {C. L.} and R. Choate and Crisler, {M. B.} and P. Cushman and R. Dixon and Dragowsky, {M. R.} and Driscoll, {D. D.} and L. Duong and J. Emes and R. Ferril and J. Filippini and Gaitskell, {R. J.} and M. Haldeman and D. Hale and D. Holmgren and Huber, {M. E.} and B. Johnson and W. Johnson and S. Kamat and M. Kozlovsky and L. Kula and S. Kyre and B. Lambin and A. Lu and R. Mahapatra and Manalaysay, {A. G.} and V. Mandic and J. May and R. McDonald and B. Merkel and P. Meunier and N. Mirabolfathi and S. Morrison and H. Nelson and R. Nelson and L. Novak and Ogburn, {R. W.} and S. Orr and Perera, {T. A.} and Isaac, {M. C.Perillo} and E. Ramberg and W. Rau and A. Reisetter and Ross, {R. R.} and T. Saab and B. Sadoulet and J. Sander and C. Savage and Schmitt, {R. L.} and Schnee, {R. W.} and Seitz, {D. N.} and B. Serfass and A. Smith and G. Smith and Spadafora, {A. L.} and K. Sundqvist and Thompson, {J. P.F.} and A. Tomada and G. Wang and J. Williams and S. Yellin and Young, {B. A.}",

note = "Funding Information: This work is supported by the National Science Foundation under Grant No. AST-9978911, by the Department of Energy under Contracts No. DE-AC03-76SF00098, No. DE-FG03-90ER40569, and No. DE-FG03-91ER40618, and by Fermilab, operated by the Universities Research Association, Inc., under Contract No. DE-AC02-76CH03000 with the Department of Energy. The ZIP detectors were fabricated in the Stanford Nanofabrication Facility operated under NSF. We are grateful to the Minnesota Department of Natural Resources and the staff of the Soudan Underground Laboratory for their assistance.",

year = "2004",

month = nov,

day = "19",

doi = "10.1103/PhysRevLett.93.211301",

language = "English (US)",

volume = "93",

journal = "Physical review letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "21",

}

TY - JOUR

T1 - First results from the cryogenic dark matter search in the soudan underground laboratory

AU - Akerib, D. S.

AU - Alvaro-Dean, J.

AU - Armel-Funkhouser, M. S.

AU - Attisha, M. J.

AU - Baudis, L.

AU - Bauer, D. A.

AU - Beaty, J.

AU - Brink, P. L.

AU - Bunker, R.

AU - Burke, S. P.

AU - Cabrera, B.

AU - Caldwell, D. O.

AU - Callahan, D.

AU - Castle, J. P.

AU - Chang, C. L.

AU - Choate, R.

AU - Crisler, M. B.

AU - Cushman, P.

AU - Dixon, R.

AU - Dragowsky, M. R.

AU - Driscoll, D. D.

AU - Duong, L.

AU - Emes, J.

AU - Ferril, R.

AU - Filippini, J.

AU - Gaitskell, R. J.

AU - Haldeman, M.

AU - Hale, D.

AU - Holmgren, D.

AU - Huber, M. E.

AU - Johnson, B.

AU - Johnson, W.

AU - Kamat, S.

AU - Kozlovsky, M.

AU - Kula, L.

AU - Kyre, S.

AU - Lambin, B.

AU - Lu, A.

AU - Mahapatra, R.

AU - Manalaysay, A. G.

AU - Mandic, V.

AU - May, J.

AU - McDonald, R.

AU - Merkel, B.

AU - Meunier, P.

AU - Mirabolfathi, N.

AU - Morrison, S.

AU - Nelson, H.

AU - Nelson, R.

AU - Novak, L.

AU - Ogburn, R. W.

AU - Orr, S.

AU - Perera, T. A.

AU - Isaac, M. C.Perillo

AU - Ramberg, E.

AU - Rau, W.

AU - Reisetter, A.

AU - Ross, R. R.

AU - Saab, T.

AU - Sadoulet, B.

AU - Sander, J.

AU - Savage, C.

AU - Schmitt, R. L.

AU - Schnee, R. W.

AU - Seitz, D. N.

AU - Serfass, B.

AU - Smith, A.

AU - Smith, G.

AU - Spadafora, A. L.

AU - Sundqvist, K.

AU - Thompson, J. P.F.

AU - Tomada, A.

AU - Wang, G.

AU - Williams, J.

AU - Yellin, S.

AU - Young, B. A.

N1 - Funding Information: This work is supported by the National Science Foundation under Grant No. AST-9978911, by the Department of Energy under Contracts No. DE-AC03-76SF00098, No. DE-FG03-90ER40569, and No. DE-FG03-91ER40618, and by Fermilab, operated by the Universities Research Association, Inc., under Contract No. DE-AC02-76CH03000 with the Department of Energy. The ZIP detectors were fabricated in the Stanford Nanofabrication Facility operated under NSF. We are grateful to the Minnesota Department of Natural Resources and the staff of the Soudan Underground Laboratory for their assistance.

PY - 2004/11/19

Y1 - 2004/11/19

N2 - The first results from the Cryogenic Dark Matter Search for weakly interacting massive particles (WIMP) in the Soudan Underground Laboratory, were investigated. Four Ge and two Si detectors were operated for about 52.6 live days, which provided 19.4 kg d of Ge net exposure after cuts for recoil energies of range between 10 and 100 keV. To define the energy threshold and selection criteria for nuclear-recoil candidates, a blind analysis was performed. These data set the world's lowest exclusion limits on the coherent WIMP-nucleon scalar cross section for all WIMP masses above 15 GeV/c 2. The results show that the minimum of this limit at the 90% C.L. is 4×10-43 cm2 at a WIMP mass of 60 GeV/c 2.

AB - The first results from the Cryogenic Dark Matter Search for weakly interacting massive particles (WIMP) in the Soudan Underground Laboratory, were investigated. Four Ge and two Si detectors were operated for about 52.6 live days, which provided 19.4 kg d of Ge net exposure after cuts for recoil energies of range between 10 and 100 keV. To define the energy threshold and selection criteria for nuclear-recoil candidates, a blind analysis was performed. These data set the world's lowest exclusion limits on the coherent WIMP-nucleon scalar cross section for all WIMP masses above 15 GeV/c 2. The results show that the minimum of this limit at the 90% C.L. is 4×10-43 cm2 at a WIMP mass of 60 GeV/c 2.

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UR - http://www.scopus.com/inward/citedby.url?scp=42749106249&partnerID=8YFLogxK

U2 - 10.1103/PhysRevLett.93.211301

DO - 10.1103/PhysRevLett.93.211301

M3 - Article

C2 - 15600991

AN - SCOPUS:42749106249

SN - 0031-9007

VL - 93

JO - Physical review letters

JF - Physical review letters

IS - 21

M1 - 211301

ER -

First results from the cryogenic dark matter search in the soudan underground laboratory

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