English

Combined Limits on WIMPs from the CDMS and EDELWEISS Experiments

Cosmology and Nongalactic Astrophysics 2015-03-19 v2 High Energy Physics - Experiment

Abstract

The CDMS and EDELWEISS collaborations have combined the results of their direct searches for dark matter using cryogenic germanium detectors. The total data set represents 614 kg.d equivalent exposure. A straightforward method of combination was chosen for its simplicity before data were exchanged between experiments. The results are interpreted in terms of limits on spin-independent WIMP-nucleon cross-section. For a WIMP mass of 90 GeV/c^2, where this analysis is most sensitive, a cross-section of 3.3 x 10^{-44} cm^2 is excluded at 90% CL. At higher WIMP masses, the combination improves the individual limits, by a factor 1.6 above 700 GeV/c^2. Alternative methods of combining the data provide stronger constraints for some ranges of WIMP masses and weaker constraints for others.

Keywords

Cite

@article{arxiv.1105.3377,
  title  = {Combined Limits on WIMPs from the CDMS and EDELWEISS Experiments},
  author = {CDMS and EDELWEISS Collaborations and : and Z. Ahmed and D. S. Akerib and E. Armengaud and S. Arrenberg and C. Augier and C. N. Bailey and D. Balakishiyeva and L. Baudis and D. A. Bauer and A. Benoît and L. Bergé and J. Blümer and P. L. Brink and A. Broniatowski and T. Bruch and V. Brudanin and R. Bunker and B. Cabrera and D. O. Caldwell and B. Censier and M. Chapellier and G. Chardin and F. Charlieux and J. Cooley and P. Coulter and G. A. Cox and P. Cushman and M. Daal and X. Defay and M. De Jesus and F. DeJongh and P. C. F. Di Stefano and Y. Dolgorouki and J. Domange and L. Dumoulin and M. R. Dragowsky and K. Eitel and S. Fallows and E. Figueroa-Feliciano and J. Filippini and D. Filosofov and N. Fourches and J. Fox and M. Fritts and J. Gascon and G. Gerbier and J. Gironnet and S. R. Golwala and M. Gros and J. Hall and R. Hennings-Yeomans and S. Henry and S. A. Hertel and S. Hervé and D. Holmgren and L. Hsu and M. E. Huber and A. Juillard and O. Kamaev and M. Kiveni and H. Kluck and M. Kos and V. Kozlov and H. Kraus and V. A. Kudryavtsev and S. W. Leman and S. Liu and P. Loaiza and R. Mahapatra and V. Mandic and S. Marnieros and C. Martinez and K. A. McCarthy and N. Mirabolfathi and D. Moore and P. Nadeau and X-F. Navick and H. Nelson and C. Nones and R. W. Ogburn and E. Olivieri and P. Pari and L. Pattavina and B. Paul and A. Phipps and M. Pyle and X. Qiu and W. Rau and A. Reisetter and Y. Ricci and M. Robinson and S. Rozov and T. Saab and B. Sadoulet and J. Sander and V. Sanglard and B. Schmidt and R. W. Schnee and S. Scorza and D. N. Seitz and S. Semikh and B. Serfass and K. M. Sundqvist and M. Tarka and A. S. Torrento-Coello and L. Vagneron and M. -A. Verdier and R. J. Walker and P. Wikus and E. Yakushev and S. Yellin and J. Yoo and B. A. Young and J. Zhang},
  journal= {arXiv preprint arXiv:1105.3377},
  year   = {2015}
}

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