Studies of a three-stage dark matter and neutrino observatory based on multi-ton combinations of liquid xenon and liquid argon detectors
arXiv:1107.1295 · doi:10.1016/j.astropartphys.2012.05.006
Abstract
We study a three stage dark matter and neutrino observatory based on multi-ton two-phase liquid Xe and Ar detectors with sufficiently low backgrounds to be sensitive to WIMP dark matter interaction cross sections down to 10E-47 cm^2, and to provide both identification and two independent measurements of the WIMP mass through the use of the two target elements in a 5:1 mass ratio, giving an expected similarity of event numbers. The same detection systems will also allow measurement of the pp solar neutrino spectrum, the neutrino flux and temperature from a Galactic supernova, and neutrinoless double beta decay of 136Xe to the lifetime level of 10E27 - 10E28 y corresponding to the Majorana mass predicted from current neutrino oscillation data. The proposed scheme would be operated in three stages G2, G3, G4, beginning with fiducial masses 1-ton Xe + 5-ton Ar (G2), progressing to 10-ton Xe + 50-ton Ar (G3) then, dependent on results and performance of the latter, expandable to 100-ton Xe + 500-ton Ar (G4). This method of scale-up offers the advantage of utilizing the Ar vessel and ancillary systems of one stage for the Xe detector of the succeeding stage, requiring only one new detector vessel at each stage. Simulations show the feasibility of reducing or rejecting all external and internal background levels to a level <1 events per year for each succeeding mass level, by utilizing an increasing outer thickness of target material as self-shielding. The system would, with increasing mass scale, become increasingly sensitive to annual signal modulation, the agreement of Xe and Ar results confirming the Galactic origin of the signal. Dark matter sensitivities for spin-dependent and inelastic interactions are also included, and we conclude with a discussion of possible further gains from the use of Xe/Ar mixtures.
References in corpus (22)
- Double Beta Decay, Majorana Neutrinos, and Neutrino Mass
- First results from DAMA/LIBRA and the combined results with DAMA/NaI
- Results from a Search for Light-Mass Dark Matter with a P-type Point Contact Germanium Detector
- Dark Matter Results from 100 Live Days of XENON100 Data
- Results from 730 kg days of the CRESST-II Dark Matter Search
- The RAVE Survey: Constraining the Local Galactic Escape Speed
- Results from a Low-Energy Analysis of the CDMS II Germanium Data
- First Dark Matter Results from the XENON100 Experiment
- The DAMA/LIBRA apparatus
- The XENON100 Dark Matter Experiment
- First results from a Dark Matter search with liquid Argon at 87 K in the Gran Sasso Underground Laboratory
- Results from the First Science Run of the ZEPLIN-III Dark Matter Search Experiment
- First limits on WIMP nuclear recoil signals in ZEPLIN-II: a two phase xenon detector for dark matter detection
- WIMP-nucleon cross-section results from the second science run of ZEPLIN-III
- Low-threshold analysis of CDMS shallow-site data
- The 2010 Interim Report of the Long-Baseline Neutrino Experiment Collaboration Physics Working Groups
- Limits on the spin-dependent WIMP-nucleon cross-sections from the first science run of the ZEPLIN-III experiment
- Coherent Neutrino Scattering in Dark Matter Detectors
- A coherent understanding of low-energy nuclear recoils in liquid xenon
- XAX: a multi-ton, multi-target detection system for dark matter, double beta decay and pp solar neutrinos
- Characterization of the QUartz Photon Intensifying Detector (QUPID) for Noble Liquid Detectors
- Discovery of underground argon with low level of radioactive 39Ar and possible applications to WIMP dark matter detectors
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- The Dawn of FIMP Dark Matter: A Review of Models and Constraints
- Snowmass CF1 Summary: WIMP Dark Matter Direct Detection
- Characterization of the Hamamatsu R11410-10 3-Inch Photomultiplier Tube for Liquid Xenon Dark Matter Direct Detection Experiments
- Expected Sensitivity to Galactic/Solar Axions and Bosonic Super-WIMPs based on the Axio-electric Effect in Liquid Xenon Dark Matter Detectors
- Reconstructing Non-standard Cosmologies with Dark Matter
- Electroweakly-Interacting Dirac Dark Matter
- Observing supernova neutrino light curve in future dark matter detectors
- A New Analysis Method for WIMP searches with Dual-Phase Liquid Xe TPCs
- The Methods for Direct Detection of WIMP with Mass <0.5 GeV
- Preliminary test results of LAr prototype detector
- State of the Art in Direct Dark Matter Detectors: Technologies, Performance, and Future Directions