Search for weakly interacting massive particles with the first five-tower data from the cryogenic dark matter search at the soudan underground laboratory.

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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DOI：
10.1103/physrevlett.102.011301
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发表时间：
2008-02
期刊：
Physical review letters
影响因子：
8.6
通讯作者：
Z. Ahmed;D. Akerib;S. Arrenberg;M. Attisha;C. N. Bailey;L. Baudis;D. Bauer;J. Beaty;P. Brink;T. Bruch;R. Bunker;S. Burke;B. Cabrera;D. Caldwell;J. Cooley;P. Cushman;F. Dejongh;M. Dragowsky;L. Duong;J. Emes;E. Figueroa-Feliciano;J. Filippini;M. Fritts;R. Gaitskell;S. Golwala;D. Grant;J. Hall;R. Hennings-Yeomans;S. Hertel;D. Holmgren;M. Huber;R. Mahapatra;V. Mandic;K. 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. Schnee;D. Seitz;B. Serfass;A. Sirois;K. Sundqvist;M. Tarka;A. Tomada;G. Wang;S. Yellin;J. Yoo;B. Young
Z. Ahmed;D. Akerib;S. Arrenberg;M. Attisha;C. N. Bailey;L. Baudis;D. Bauer;J. Beaty;P. Brink;T. Bruch;R. Bunker;S. Burke;B. Cabrera;D. Caldwell;J. Cooley;P. Cushman;F. Dejongh;M. Dragowsky;L. Duong;J. Emes;E. Figueroa-Feliciano;J. Filippini;M. Fritts;R. Gaitskell;S. Golwala;D. Grant;J. Hall;R. Hennings-Yeomans;S. Hertel;D. Holmgren;M. Huber;R. Mahapatra;V. Mandic;K. 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. Schnee;D. Seitz;B. Serfass;A. Sirois;K. Sundqvist;M. Tarka;A. Tomada;G. Wang;S. Yellin;J. Yoo;B. Young
中科院分区：
物理与天体物理1区
文献类型：
--
作者：
Z. Ahmed;D. Akerib;S. Arrenberg;M. Attisha;C. N. Bailey;L. Baudis;D. Bauer;J. Beaty;P. Brink;T. Bruch;R. Bunker;S. Burke;B. Cabrera;D. Caldwell;J. Cooley;P. Cushman;F. Dejongh;M. Dragowsky;L. Duong;J. Emes;E. Figueroa-Feliciano;J. Filippini;M. Fritts;R. Gaitskell;S. Golwala;D. Grant;J. Hall;R. Hennings-Yeomans;S. Hertel;D. Holmgren;M. Huber;R. Mahapatra;V. Mandic;K. 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. Schnee;D. Seitz;B. Serfass;A. Sirois;K. Sundqvist;M. Tarka;A. Tomada;G. Wang;S. Yellin;J. Yoo;B. Young

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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 6.6x10;{-44} cm;{2} (4.6x10;{-44} cm;{2} when combined with previous CDMS II data) at the 90% confidence level for a WIMP mass of 60 GeV/c;{2}. This achieves the best sensitivity for dark matter WIMPs with masses above 44 GeV/c;{2}, and significantly restricts the parameter space for some favored supersymmetric models.