First results from a dark matter search with liquid argon at 87 K in the Gran Sasso underground laboratory

Abstract A new method of searching for dark matter in the form of weakly interacting massive particles (WIMP) has been developed with the direct detection of the low energy nuclear recoils observed in a massive target (ultimately many tons) of ultra pure liquid argon at 87 K. A high selectivity for argon recoils is achieved by the simultaneous observation of both the VUV scintillation luminescence and of the electron signal surviving columnar recombination, extracted through the liquid–gas boundary by an electric field. First physics results from this method are reported, based on a small 2.3 l test chamber filled with natural argon and an accumulated fiducial exposure of about 100 kg day, supporting the future validity of this method with isotopically purified 40Ar and for a much larger unit presently under construction with correspondingly increased sensitivities.

[1]  L. Schoeffel,et al.  Final results of the EDELWEISS-I dark matter search with cryogenic heat-and-ionization Ge detectors , 2005, astro-ph/0503265.

[2]  S. Kubota,et al.  Dynamical behavior of free electrons in the recombination process in liquid argon, krypton, and xenon , 1979 .

[3]  E. Mazor,et al.  Natural gas association with water and oil as depicted by atmospheric noble gases: case studies from the southeastern Mediterranean Coastal Plain , 1988 .

[4]  H. Loosli A dating method with39Ar , 1983 .

[5]  E. R. Oxburgh,et al.  Rare gas constraints on hydrocarbon accumulation, crustal degassing and groundwater flow in the Pannonian Basin , 1991 .

[6]  Lukas A. Schaller,et al.  Nuclear ground state charge radii from electromagnetic interactions , 1995 .

[7]  WMAP constraints on SUGRA models with non-universal gaugino masses and prospects for direct detection , 2004, hep-ph/0407218.

[8]  G. Wasserburg,et al.  Helium, argon, and carbon in some natural gases , 1961 .

[9]  P. Benetti,et al.  Detection of the VUV liquid argon scintillation light by means of glass-window photomultiplier tubes , 2003 .

[10]  Goodman,et al.  Detectability of certain dark-matter candidates. , 1985, Physical review. D, Particles and fields.

[11]  David J. Thomas,et al.  High resolution measurements of neutron energy spectra from AmBe and AmB neutron sources , 1995 .

[12]  A. Hitachi,et al.  Effect of ionization density on the time dependence of luminescence from liquid argon and xenon , 1983 .

[13]  S. Weinberg,et al.  Cosmological lower bound on heavy-neutrino masses , 1977 .

[14]  V. A. Kudryavtsev,et al.  Low energy neutron propagation in MCNPX and GEANT4 , 2006 .

[15]  J. Keto,et al.  Exciton lifetimes in electron beam excited condensed phases of argon and xenon , 1979 .

[16]  Lars Bergström,et al.  Non-baryonic dark matter: observational evidence and detection methods , 2000 .

[17]  S. Amerio,et al.  Design, construction and tests of the ICARUS T600 detector , 2004 .

[18]  A. Reisetter Results from the Cryogenic Dark Matter Search Experiment , 2003 .

[19]  R. Spangler,et al.  Noble gas and methane partitioning from ground water: An aid to natural gas exploration and reservoir evaluation , 1990 .

[20]  B. Lollar,et al.  Regional groundwater focusing of nitrogen and noble gases into the Hugoton-Panhandle giant gas field, USA , 2002 .

[21]  J. Magee,et al.  TRIPLET FORMATION IN ION RECOMBINATION IN SPURS. , 1972 .

[22]  J. B. Birks,et al.  The Theory and Practice of Scintillation Counting , 1965 .

[23]  G. J. Alner,et al.  First limits on nuclear recoil events from the ZEPLIN I galactic dark , 2005 .

[24]  A. Hime,et al.  Technique for direct detection of weakly interacting massive particles using scintillation time discrimination in liquid argon , 2006 .

[25]  S. Kubota,et al.  Variation of scintillation decay in liquid argon excited by electrons and alpha particles , 1978 .

[26]  J. Engel Nuclear form factors for the scattering of weakly interacting massive particles , 1991 .

[27]  J. P. Castle,et al.  Exclusion Limits on the WIMP Nucleon Cross-Section from the Cryogenic Dark Matter Search , 2002 .

[28]  J. Ellis,et al.  Direct detection of dark matter in the minimal supersymmetric standard model with non-universal Higgs boson masses , 2003 .

[29]  T. Suemoto,et al.  Time-Resolved Absorption Spectroscopy of Self-Trapped Excitons in Condensed Ne, Ar, and Kr , 1979 .

[30]  L. Stodolsky,et al.  Limits on WIMP dark matter using scintillating CaWO4 cryogenic detectors with active background suppression , 2004, astro-ph/0408006.

[31]  F. Donato,et al.  Light neutralinos and WIMP direct searches , 2003, hep-ph/0307303.

[32]  P. Belli,et al.  Search for WIMP annual modulation signature: Results from DAMA/NaI-3 and DAMA/NaI-4 and the global combined analysis , 2000 .

[33]  Ursula Curtiss,et al.  Letter of intent , 1971 .

[34]  Improved exclusion limits from the edelweiss wimp search , 2002, astro-ph/0206271.

[35]  A. Bottino,et al.  Probing the supersymmetric parameter space by weakly interacting massive particle direct detection , 2001 .

[36]  J. Schijf,et al.  Geochimica et Cosmochimica Acta , 2008 .

[37]  J. P. Castle,et al.  First results from the Cryogenic Dark Matter Search in the Soudan Underground Laboratory. , 2004, Physical review letters.