The SIMPLE Phase II dark matter search

M. Felizardo, T. A. Girard, T. Morlat, A. C. Fernandes, A. R. Ramos, J. G. Marques, A. Kling, J. Puibasset, M. Auguste, D. Boyer, A. Cavaillou, J. Poupeney, C. Sudre, F. P. Carvalho, M. I. Prudêncio, and R. Marques
Phys. Rev. D 89, 072013 – Published 22 April 2014

Abstract

Phase II of SIMPLE (Superheated Instrument for Massive ParticLe Experiments) searched for astroparticle dark matter using superheated liquid C2ClF5 droplet detectors. Each droplet generally requires an energy deposition with linear energy transfer (LET) 150keV/μm for a liquid-to-gas phase transition, providing an intrinsic rejection against minimum ionizing particles of order 1010, and reducing the backgrounds to primarily α and neutron-induced recoil events. The droplet phase transition generates a millimetric-sized gas bubble that is recorded by acoustic means. We describe the SIMPLE detectors, their acoustic instrumentation, and the characterizations, signal analysis and data selection, which yield a particle-induced, “true nucleation” event detection efficiency of better than 97% at a 95% C.L. The recoil-α event discrimination, determined using detectors first irradiated with neutrons and then doped with alpha emitters, provides a recoil identification of better than 99%; it differs from those of COUPP and PICASSO primarily as a result of their different liquids with lower critical LETs. The science measurements, comprising two shielded arrays of fifteen detectors each and a total exposure of 27.77 kgd, are detailed. Removal of the 1.94 kgd Stage 1 installation period data, which had previously been mistakenly included in the data, reduces the science exposure from 20.18 to 18.24 kgd and provides new contour minima of σp=4.3×103pb at 35GeV/c2 in the spin-dependent sector of astroparticle dark matter–proton interactions and σN=3.6×106pb at 35GeV/c2 in the spin-independent sector. These results are examined with respect to the fluorine spin and halo parameters used in the previous data analysis.

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  • Received 19 September 2013

DOI:https://doi.org/10.1103/PhysRevD.89.072013

© 2014 American Physical Society

Authors & Affiliations

M. Felizardo1,2,3, T. A. Girard2,4,*, T. Morlat5, A. C. Fernandes2,3, A. R. Ramos2,3, J. G. Marques2,3, A. Kling2,3, J. Puibasset6, M. Auguste7, D. Boyer7, A. Cavaillou7, J. Poupeney7, C. Sudre7, F. P. Carvalho3, M. I. Prudêncio3, and R. Marques3

  • 1Department of Physics, Universidade Nova de Lisboa, 2829-516 Caparica, Portugal
  • 2Centro de Física Nuclear, Universidade de Lisboa, 1649-003 Lisbon, Portugal
  • 3Instituto Tecnológico e Nuclear, IST, Universidade Técnica de Lisboa, EN 10, 2686-953 Sacavém, Portugal
  • 4Department of Physics, Universidade Lisboa, 1749-016 Lisbon, Portugal
  • 5Ecole Normale Superieur de Montrouge, 1 Rue Aurice Arnoux, 92120 Montrouge, France
  • 6Centre de Recherche sur la Matière Divisée, CNRS, Université de Orléans, 45071 Orléans, France
  • 7Laboratoire Souterrain à Bas Bruit (UMS 3538 UNS/UAPV/CNRS), 84400 Rustrel–Pays d’Apt, France

  • *criodets@cii.fc.ul.pt

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Vol. 89, Iss. 7 — 1 April 2014

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