The XENON Dark Matter Search Experiment

E. Aprile; K. L. Giboni; P. Majewski; K. Ni; M. Yamashita; R. Gaitskell; P. Sorensen; L. DeViveiros; L. Baudis; A. Bernstein; C. Hagmann; C. Winant; T. Shutt; J. Kwong; U. Oberlack; D. McKinsey; R. Hasty

doi:10.1016/j.newar.2005.01.035

arXiv · astro-ph/0407575

The XENON Dark Matter Search Experiment

E. Aprile·K. L. Giboni·P. Majewski·K. Ni·M. Yamashita·R. Gaitskell·P. Sorensen·L. DeViveiros·L. Baudis·A. Bernstein·C. Hagmann·C. Winant·T. Shutt·J. Kwong·U. Oberlack·D. McKinsey·R. Hasty

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Abstract

The XENON experiment aims at the direct detection of dark matter in the form of WIMPs (Weakly Interacting Massive Particles) via their elastic scattering off Xe nuclei. A fiducial mass of 1000 kg, distributed in ten independent liquid xenon time projection chambers(LXeTPCs) will be used to probe thelowest interaction cross section predicted by SUSY models. The TPCs are operated in dual (liquid/gas) phase, to allow a measurement of nuclear recoils down to 16keV energy, via simultaneous detection of the ionization, through secondary scintillation in the gas, and primary scintillation in the liquid. Thedistinct ratio of primary to secondary scintillation for nuclear recoils from WIMPs (or neutrons), and for electron recoils from background, iskey to the event-by-event discrimination capability of XENON. A dual phase xenon prototype has been realized and is currently being tested, along with otherprototypes dedicated to other measurements relevant to the XENON program. As part of the R&D phase, we will realize and move underground a first XENON module (XENON10) with at least 10 kg fiducial mass to measure the background rejection capability and to optimize the conditions for continuous and stable detector operation underground. We present some of the results from the ongoing R&D and summarize the expected performance of the 10 kg experiment, from MonteCarlo simulations. The main design features of the 100 kg detector unit(XENON100), with which we envisage to make up the 1 tonne sensitive mass ofXENON1T will also be presented.

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E. Aprile, K. L. Giboni, P. Majewski, K. Ni, M. Yamashita, R. Gaitskell, P. Sorensen, L. DeViveiros, L. Baudis, A. Bernstein, C. Hagmann, C. Winant, T. Shutt, J. Kwong, U. Oberlack, D. McKinsey, R. Hasty. 2004-07-28. The XENON Dark Matter Search Experiment. https://doi.org/10.1016/j.newar.2005.01.035

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