xenon.physics.rice.edu
XENON - Dark Matter SearchXENON Dark Matter Search at the High Energy and Particle Astrophysics Lab @ Rice
http://xenon.physics.rice.edu/
XENON Dark Matter Search at the High Energy and Particle Astrophysics Lab @ Rice
http://xenon.physics.rice.edu/
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XENON - Dark Matter Search | xenon.physics.rice.edu Reviews
https://xenon.physics.rice.edu
XENON Dark Matter Search at the High Energy and Particle Astrophysics Lab @ Rice
xenon.physics.rice.edu
Dark Matter
http://xenon.physics.rice.edu/dm.html
Dark Matter XENON Detector. Evidence for Dark Matter. Today, we have striking astrophysical evidence that Dark Matter really exists. This is matter that is not made out of the particles described by the Standard Model of Particle Physics. It does not emit any kind of radiation (therefore we cannot "see" it), and probably interacts only via the weak interaction. However, it has a finite mass and can be detected due to the associated gravitational force. Some of the evidences for Dark Matter are:. This ide...
XENON - Collaboration
http://xenon.physics.rice.edu/collaboration.html
Members of the XENON100 Collaboration. The XENON100 collaboration: Collaboration meeting at LNGS, October 20-21, 2007. Elena Aprile, Bin Choi, Karl-Ludwig Giboni, Rafael Lang, Kyungeun Lim, Antonio Melgarejo, Kaixuan Ni, Guillaume Plante. Uwe Oberlack, Yuan Mei, Peter Shagin. University Zurich, Switzerland. Laura Baudis, Ali Askin, Annika Behrens, Alfredo Ferella, Alexander Kish, Roberto Santorelli, Marc Schumann, Teresa Marrodan Undagoitia. Gran Sasso National Laboratory, Italy. M Lindner, H. Simgen.
XENON100
http://xenon.physics.rice.edu/xenon100.html
XENON100 - The next Step towards 1 Ton. After the very successful run of XENON10. The first XENON detector with an overall mass of 15 kg and a target mass of 5.4 kg (after cuts), a part of the collaboration decided to go one step further: XENON100. Will have a 10 times larger fiducial volume. This will increase the sensitivity to the WIMP parameter space even further and will provide an improved chance to detect WIMPs directly. Rice's Contribution to XENON100. Prototype of a XENON 100 TPC anode grid.
The XENON Detector
http://xenon.physics.rice.edu/detector.html
An experiment that is designed to successfully detect new particles with extremely low interaction probabilities - the Dark Matter WIMPs - has to fulfill several criteria. Some of them are:. The experiment has to be performed in a low background environment, i.e. in underground laboratories located under mountains or in deep mines. Internal radioactivity (from detector components, housing, etc.) must be small. The noble gas xenon is a perfect target material: It can be purified very effectively on the pa...
XENON - Dark Matter Search :: Photo Gallery
http://xenon.physics.rice.edu/gallery.html
M Schumann, U. Oberlack, and P. Shagin (Rice) and the XENON100 TPC. The XENON100 detector assembly in the cleanroom. The Top PMT array with 99 1"x1" PMTs after assembly. A Kish (Zurich) working on the XENON100 TPC. KE Lim (Columbia) with the bottom PMT array (80 PMTs). R Santorelli (Zurich), G. Plante (Columbia), S. Fattori (LNGS), and E. Tziaferi (Zurich). Detail of the bottom veto PMTs on the fully assembled TPC. Relaxing on a Sunday trip to the wonderful Italian countryside. Pictures courtesy of sever...
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Group Members
http://astroparticlelab.rice.edu/group.html
Dept of Physics and Astronomy. 6100 Main St., MS 108. Houston, TX 77005-1827. Fax : 1 713-348-3690. Dept of Physics and Astronomy. 6100 Main St., MS 108. Houston, TX 77005-1827. Fax : 1 713-348-3690. Dept of Physics and Astronomy. 6100 Main St., MS 108. Houston, TX 77005-1827. Fax : 1 713-348-3690. E-mail: richard.a.wall(at)rice.edu.
Gamma Ray Astronomy
http://astroparticlelab.rice.edu/gamma.html
Gamma Ray Astronomy XENON. Uwe Oberlack has moved to Johannes Gutenberg University, Mainz, Germany. For more information, please look here. Past work: For more information please check these. P Shagin, R. Gomez, U.G. Oberlack, P. Cushmann, B. Sherwood, M. McClish, R. Farrell. Test of Avalanche Photodiodes for Liquid Xenon Scintillation: Quantum Efficiency and Gain. JINST 4 P01005 (2009). E Aprile, A. Curioni, K.L. Giboni, M. Kobayashi, U.G. Oberlack, S. Zhang,. Nucl Instr. Meth. A 593, 414 (2008).
The XENON Dark Matter Project
http://xenon.astro.columbia.edu/XENON100_Experiment/Collaboration
The XENON Dark Matter Project. The XENON Project Home. Dark Matter Limit Plot. Dark Matter Online Tools. Columbia University, USA. Rice University, USA. University of California, Los Angeles, USA. University of Zurich, Switzerland. University of Coimbra, Portugal. Gran Sasso National Laboratories, Italy. INFN Turin, Italy. Shanghai Jiao Tong University, China. Johannes Gutenberg University Mainz, Germany. University of Bologna, Italy. University of Müenster, Germany. Weizmann Institute of Science, Israel.
Job Openings
http://astroparticlelab.rice.edu/jobs.html
These jobs are currently available in the High Energy and Particle Astrophysics Lab:. For information and application please contact:. Dept of Physics and Astronomy. 6100 Main St., MS 108. Houston, TX 77005-1827. Fax : 1 713-348-3690.
Internal Sites
http://astroparticlelab.rice.edu/internal.html
Internal Sites @ Rice. The following password protected internal sites are available:. Internal Rice group site. Updated: 09/23/2007 by Marc Schumann.
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XENON - Dark Matter Search
XENON100 released spin-dependent WIMP-nucleon cross sections limits from 225 live days data. July 9, 2013:. The XENON100 collaboration submitted a paper with the limits of spin-dependent WIMP-nucleon cross sections from a 225 live days data to PRL, setting the most stringent upper limits on WIMP-neutron cross sections for WIMP masses above 6 GeV. The preprint can be found here: arXiv:1301.6620. XENON100 released 225 live days results. July 25, 2012:. The preprint can be found here: arXiv:1207.5988. Due t...
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