Improved spin-dependent limits from the PICASSO dark matter search experiment
The PICASSO experiment reports an improved limit for the existence of cold dark matter WIMPs interacting via spin-dependent interactions with nuclei. The experiment is installed in the Sudbury Neutrino Observatory at a depth of 2070 m. With superheated C4F10 droplets as the active material, and an e...
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| Published in | Physics letters. B Vol. 624; no. 3-4; pp. 186 - 194 |
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| Main Authors | , , , , , , , , , , , , , , , , , , , |
| Format | Journal Article |
| Language | English |
| Published |
Amsterdam
Elsevier B.V
29.09.2005
Elsevier Science |
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| Abstract | The PICASSO experiment reports an improved limit for the existence of cold dark matter WIMPs interacting via spin-dependent interactions with nuclei. The experiment is installed in the Sudbury Neutrino Observatory at a depth of 2070 m. With superheated C4F10 droplets as the active material, and an exposure of 1.98±0.19 kg day, no evidence for a WIMP signal was found. For a WIMP mass of 29 GeV/c2, limits on the spin-dependent cross section on protons of σp=1.31 pb and on neutrons of σn=21.5 pb have been obtained at 90% C.L. In both cases, some new parameter space in the region of WIMP masses below 20 GeV/c2 has now been ruled out. The results of these measurements are also presented in terms of limits on the effective WIMP-proton and neutron coupling strengths ap and an. |
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| AbstractList | The PICASSO experiment reports an improved limit for the existence of cold dark matter WIMPs interacting via spin-dependent interactions with nuclei. The experiment is installed in the Sudbury Neutrino Observatory at a depth of 2070 m. With superheated C4F10 droplets as the active material, and an exposure of 1.98±0.19 kg day, no evidence for a WIMP signal was found. For a WIMP mass of 29 GeV/c2, limits on the spin-dependent cross section on protons of σp=1.31 pb and on neutrons of σn=21.5 pb have been obtained at 90% C.L. In both cases, some new parameter space in the region of WIMP masses below 20 GeV/c2 has now been ruled out. The results of these measurements are also presented in terms of limits on the effective WIMP-proton and neutron coupling strengths ap and an. |
| Author | Levine, I. Wichoski, U. Martin, J.-P. Feighery, W. Muthusi, C. Kanagalingam, S. Guénette, R. Barnabé-Heider, M. Noulty, R. Clark, K. Lessard, L. Behnke, E. Gornea, R. Zacek, V. Krauss, C. Noble, A. Leroy, C. Genest, M.-H. Doane, P. Di Marco, M. |
| Author_xml | – sequence: 1 givenname: M. surname: Barnabé-Heider fullname: Barnabé-Heider, M. organization: Département de Physique, Université de Montréal, Montréal, H3C 3J7, Canada – sequence: 2 givenname: M. surname: Di Marco fullname: Di Marco, M. organization: Département de Physique, Université de Montréal, Montréal, H3C 3J7, Canada – sequence: 3 givenname: P. surname: Doane fullname: Doane, P. organization: Département de Physique, Université de Montréal, Montréal, H3C 3J7, Canada – sequence: 4 givenname: M.-H. surname: Genest fullname: Genest, M.-H. organization: Département de Physique, Université de Montréal, Montréal, H3C 3J7, Canada – sequence: 5 givenname: R. surname: Gornea fullname: Gornea, R. organization: Département de Physique, Université de Montréal, Montréal, H3C 3J7, Canada – sequence: 6 givenname: R. surname: Guénette fullname: Guénette, R. organization: Département de Physique, Université de Montréal, Montréal, H3C 3J7, Canada – sequence: 7 givenname: C. surname: Leroy fullname: Leroy, C. organization: Département de Physique, Université de Montréal, Montréal, H3C 3J7, Canada – sequence: 8 givenname: L. surname: Lessard fullname: Lessard, L. organization: Département de Physique, Université de Montréal, Montréal, H3C 3J7, Canada – sequence: 9 givenname: J.-P. surname: Martin fullname: Martin, J.-P. organization: Département de Physique, Université de Montréal, Montréal, H3C 3J7, Canada – sequence: 10 givenname: U. surname: Wichoski fullname: Wichoski, U. organization: Département de Physique, Université de Montréal, Montréal, H3C 3J7, Canada – sequence: 11 givenname: V. surname: Zacek fullname: Zacek, V. email: zacekv@lps.umontreal.ca organization: Département de Physique, Université de Montréal, Montréal, H3C 3J7, Canada – sequence: 12 givenname: K. surname: Clark fullname: Clark, K. organization: Department of Physics, Queens University, Kingston, K7L 3NG, Canada – sequence: 13 givenname: C. surname: Krauss fullname: Krauss, C. organization: Department of Physics, Queens University, Kingston, K7L 3NG, Canada – sequence: 14 givenname: A. surname: Noble fullname: Noble, A. organization: Department of Physics, Queens University, Kingston, K7L 3NG, Canada – sequence: 15 givenname: E. surname: Behnke fullname: Behnke, E. organization: Departments of Physics & Astronomy, Indiana University South Bend, South Bend, IN 46634, USA – sequence: 16 givenname: W. surname: Feighery fullname: Feighery, W. organization: Chemistry, Indiana University South Bend, South Bend, IN 46634, USA – sequence: 17 givenname: I. surname: Levine fullname: Levine, I. organization: Departments of Physics & Astronomy, Indiana University South Bend, South Bend, IN 46634, USA – sequence: 18 givenname: C. surname: Muthusi fullname: Muthusi, C. organization: Chemistry, Indiana University South Bend, South Bend, IN 46634, USA – sequence: 19 givenname: S. surname: Kanagalingam fullname: Kanagalingam, S. organization: Bubble Technology Industries, Chalk River, K0J 1J0, Canada – sequence: 20 givenname: R. surname: Noulty fullname: Noulty, R. organization: Bubble Technology Industries, Chalk River, K0J 1J0, Canada |
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| Cites_doi | 10.1063/1.1724333 10.1016/0029-554X(79)90735-3 10.1016/S0168-9002(02)01925-3 10.1016/j.physletb.2004.01.092 10.1016/S1350-4487(96)00156-4 10.1016/S0370-2693(00)00846-7 10.1016/S0927-6505(96)00047-3 10.1103/PhysRevD.40.2131 10.1016/0370-2693(91)90597-J 10.1103/PhysRev.87.665 10.1103/PhysRevLett.85.3083 10.1103/PhysRevD.55.503 10.1109/23.819251 10.1103/PhysRevLett.93.161301 10.1007/BF02781560 10.1016/S0927-6505(00)00123-7 10.1016/S0168-9002(97)00074-0 |
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| Keywords | Protons Weak interactions Dark matter Cold dark matter Sudbury neutrino observatory Neutrons Massive particle Droplets Cross sections |
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