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Cited by 648

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First Results from the XENON10 Dark Matter Experiment at the Gran Sasso National Laboratory

Open access
Angle, J., Aprile, E., Arneodo, F., Baudis, L., Bernstein, A., Bolozdynya, A., Brusov, P., Coelho, L. C. C., Dahl, C. E., DeViveiros, L., Ferella, A. D., Fernandes, L. M. P., Fiorucci, S., Gaitskell, R. J., Giboni, K. L., Gomez, R., Hasty, R., Kastens, L., Kwong, J., Lopes, J. A. M., Madden, N., Manalaysay, A., Manzur, A., McKinsey, D. N., Monzani, M. E., Ni, K., Oberlack, U., Orboeck, J., Plante, G., Santorelli, R., dos Santos, J. M. F., Shagin, P., Shutt, T., Sorensen, P., Schulte, S., Winant, C., Yamashita, M.·2008·Physical Review Letters

Abstract

The XENON10 experiment at the Gran Sasso National Laboratory uses a 15 kg xenon dual phase time projection chamber to search for dark matter weakly interacting massive particles (WIMPs). The detector measures simultaneously the scintillation and the ionization produced by radiation in pure liquid xenon to discriminate signal from background down to 4.5 keV nuclear-recoil energy. A blind analysis of 58.6 live days of data, acquired between October 6, 2006, and February 14, 2007, and using a fiducial mass of 5.4 kg, excludes previously unexplored parameter space, setting a new 90% C.L. upper limit for the WIMP-nucleon spin-independent cross section of $8.8\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}44}\text{ }\text{ }{\mathrm{cm}}^{2}$ for a WIMP mass of $100\text{ }\text{ }\mathrm{GeV}/{c}^{2}$, and $4.5\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}44}\text{ }\text{ }{\mathrm{cm}}^{2}$ for a WIMP mass of $30\text{ }\text{ }\mathrm{GeV}/{c}^{2}$. This result further constrains predictions of supersymmetric models.

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Metadata

Authors
Angle, J., Aprile, E., Arneodo, F., Baudis, L., Bernstein, A., Bolozdynya, A., Brusov, P., Coelho, L. C. C., Dahl, C. E., DeViveiros, L., Ferella, A. D., Fernandes, L. M. P., Fiorucci, S., Gaitskell, R. J., Giboni, K. L., Gomez, R., Hasty, R., Kastens, L., Kwong, J., Lopes, J. A. M., Madden, N., Manalaysay, A., Manzur, A., McKinsey, D. N., Monzani, M. E., Ni, K., Oberlack, U., Orboeck, J., Plante, G., Santorelli, R., dos Santos, J. M. F., Shagin, P., Shutt, T., Sorensen, P., Schulte, S., Winant, C., & Yamashita, M.
Venue
Physical Review Letters
Published
2008-01-17
Volume
100
Issue
2
Pages
021303-021303
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2006441137
Cited by
648
References
18
FWCI
79.33
Type
journal article
Language
en
Open access
green

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Angle, J., Aprile, E., Arneodo, F., Baudis, L., Bernstein, A., Bolozdynya, A., Brusov, P., Coelho, L. C. C., Dahl, C. E., DeViveiros, L., Ferella, A. D., Fernandes, L. M. P., Fiorucci, S., Gaitskell, R. J., Giboni, K. L., Gomez, R., Hasty, R., Kastens, L., Kwong, J., . . . Yamashita, M. (2008). First Results from the XENON10 Dark Matter Experiment at the Gran Sasso National Laboratory. Physical Review Letters. https://doi.org/10.1103/physrevlett.100.021303

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