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A study of the trace 39Ar content in argon from deep underground sources
Affiliation:1. Department of Physics, Princeton University, Princeton NJ 08544, USA;2. INFN Laboratori Nazionali del Gran Sasso, SS 17 bis Km 18_910, 067010 Assergi (AQ), Italy;3. Physics Department, Temple University, Philadelphia, PA 19122, USA;4. Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA 02138, USA;5. Physics Department, Virginia Polytechnic Institute and State University, Blacksburg, VA 24061, USA;1. Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics, Stanford University and SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, CA 94025, USA;2. Institute for Nuclear Research, 60th October Anniversary Prospect 7a, Moscow 117312, Russia;3. Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547, USA;4. Kavli IPMU (WPI), University of Tokyo, Kashiwa, Chiba 277-8568, Japan;1. Department of Physics, University of Alberta, Edmonton, Alberta T6G 2R3, Canada;2. Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1, Canada;3. Chemistry Department, Brookhaven National Laboratory, Upton, NY 11973-5000, United States;4. Ottawa-Carleton Institute for Physics, Department of Physics, Carleton University, Ottawa, Ontario K1S 5B6, Canada;5. Physics Department, University of Guelph, Guelph, Ontario N1G 2W1, Canada;6. Department of Physics and Astronomy, Laurentian University, Sudbury, Ontario P3E 2C6, Canada;7. Institute for Nuclear and Particle Astrophysics and Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, United States;8. Laboratório de Instrumentação e Física Experimental de Partículas, Av. Elias Garcia 14, 1°, 1000-149 Lisboa, Portugal;9. Los Alamos National Laboratory, Los Alamos, NM 87545, United States;10. Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803, United States;11. Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, MA 02139, United States;12. Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK;13. Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104-6396, United States;14. Department of Physics, Queen’s University, Kingston, Ontario K7L 3N6, Canada;15. Rutherford Appleton Laboratory, Chilton, Didcot OX11 0QX, UK;p. SNOLAB, Sudbury, ON P3Y 1M3, Canada;q. Department of Physics, University of Texas at Austin, Austin, TX 78712-0264, United States;r. TRIUMF, 4004 Wesbrook Mall, Vancouver, BC V6T 2A3, Canada;s. Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, WA 98195, United States;t. Department of Physics, University of Washington, Seattle, WA 98195, United States;1. Dipartimento di Fisica, Università degli Studi di Milano, via G. Celoria, 16, 20133 Milano, Italy;2. INFN Milano, via G. Celoria, 16, 20133 Milano, Italy;3. INFN Pavia, via A. Bassi, 6, 27100 Pavia, Italy;4. Dept. of Information Engineering, University of Padova, via Gradenigo 6/A, 35131 Padova, Italy;1. Università di Genova and INFN, Genova, Italy;2. Argonne National Laboratory, Argonne, IL, United States;3. Instituto de Física Corpuscular (IFIC), Valencia, Spain;4. Oxford University, Oxford, United Kingdom;5. Université Paris-Sud and CNRS/IN2P3, Orsay, France;6. Brookhaven National Laboratory, Upton, NY, United States;7. Universidad Técnica Federico Santa María, Valparaíso, Chile;8. CERN, Geneva, Switzerland
Abstract:
Keywords:Underground argon  Dark matter instrumentation  Low-radioactivity technique  Low-background counting
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