News
2010/09/20
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2007/04/14
XENON10 results from a 3 month WIMP search run at the Gran Sasso National Laboratory announced at the APS April Meeting. The solid red curve is the lastest XENON10 result.
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"First Dark Matter Results from the XENON100 Experiment" was published in Phys. Rev. Lett. |
2010/07/29
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"Liquid xenon detectors for particle physics and astrophysics" was published in Review of Modern Physics. |
2010/07/08
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The Discovery Interview: The Dark Hunter |
2010/05/06
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Columbia E-NEWS: Highly Sensitive Dark Matter Experiment Disproves Earlier Findings |
2010/05/04
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nature.com: Dark matter stays dark |
2010/05/03
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The New York Times: Particle Detector Shows Promise, if Nothing Else |
2010/01/16
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"Design and Performance of the XENON10 Dark Matter Experiment" is available in arXiv. |
2009/12/09
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"Constraints on inelastic dark matter from XENON10" was published in Phys. Rev. D. |
2009/08/04
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WIRED: Let there be light! The search for dark matter. |
2009/07/27
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Columbia E-NEWS: Columbia Researchers Lead Race to Find Dark Matter. |
2009/04/22
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"New Measurement of the Relative Scintillation Efficiency of Xenon Nuclear Recoils Below 10 keV" was published in Phys. Rev. C. |
2009/03/18
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"Status and Sensitivity Projections for the XENON100 Dark Matter Experiment" was accepted in Proceedings of Science (IDM2008) 018. |
2008/09/05
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"Limits on spin-dependent WIMP-nucleon cross-sections from the XENON10 experiment" was published in Phys. Rev. Lett. |
2008/07/23
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After a long waiting time, the Kr distillation column was finally delivered to LNGS. Kr-85 is one intrinsic radioactive source in Xe. The XENON100 experiment's sensitivity goal requires a Kr/Xe contamination level lower than 50 ppt. The current Kr/Xe contamination level in XENON100 is about 5 ppb. Cryogenic distillation through the new column, which will take about two weeks for the 170 kg Xe in the detector, will reduce the Kr/Xe level by three orders of magnitude, making the Kr-85 contribution to the XENON100 total background negligible. |
2008/04/20
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XENON100 Poster was presented at the APS spring meeting. It gives a good overview about XENON Program and the basics of XENON100 experiment. |
2008/02/22
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XENON100 detector construction completed. See Elena Aprile's presentation at the UCLA Dark Matter 2008 conference. |
2008/01/17
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"First Results from the XENON10 Dark Matter Experiment at the Gran Sasso National Laboratory" was published in Phys. Rev. Lett. |
2007/12/15
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Columbia University Ground Breaking Work: Elena Aprile (Physics/Applied Physics), This new device can detect dark matter, the never-found state of matter that current theory says should make up 90 percent of the universe. |
2007/11/14
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Discover: The 6 Most Important Experiments in the World |
2007/08/12
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USA Today: Researchers use high-tech machines to detect mysterious dark matter |
2007/07/18
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Nature: Unseen Universe: Welcome to the dark side |
2007/04/17
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Nature: Dark matter looks to be particularly wimpy |
2007/04/14
XENON10 results from a 3 month WIMP search run at the Gran Sasso National Laboratory announced at the APS April Meeting. The solid red curve is the lastest XENON10 result.
