Amole, C.; Ardid Ramírez, M.; Arnquist, I.; Asner, DM.; Baxter, D.; Behnke, E.; Bhattacharjee, P.... (2016). Improved dark matter search results from PICO-2L Run 2. Physical Review D. 93(6):1-5. https://doi.org/10.1103/PhysRevD.93.061101
Por favor, use este identificador para citar o enlazar este ítem: http://hdl.handle.net/10251/80316
Title:
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Improved dark matter search results from PICO-2L Run 2
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Author:
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Amole, C.
Ardid Ramírez, Miguel
Arnquist, I.J.
Asner, D. M.
Baxter, D.
Behnke, E.
Bhattacharjee, P.
Borsodi, h.
Bou Cabo, Manuel
Brice, S.J.
Broemmelsiek, D.
Clark, K.
Collar, J.I.
Cooper, P.S.
Felis Enguix, Iván
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UPV Unit:
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Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres
Universitat Politècnica de València. Escuela Técnica Superior de Ingeniería del Diseño - Escola Tècnica Superior d'Enginyeria del Disseny
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Issued date:
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Abstract:
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New data are reported from a second run of the 2-liter PICO-2L C3F8 bubble chamber with a total exposure of 129 kg-days at a thermodynamic threshold energy of 3.3 keV. These data show that measures taken to control particulate ...[+]
New data are reported from a second run of the 2-liter PICO-2L C3F8 bubble chamber with a total exposure of 129 kg-days at a thermodynamic threshold energy of 3.3 keV. These data show that measures taken to control particulate contamination in the superheated fluid resulted in the absence of the anomalous background events observed in the first run of this bubble chamber. One single nuclear-recoil event was observed in the data, consistent both with the predicted background rate from neutrons and with the observed rate of unambiguous multiple-bubble neutron scattering events. The chamber exhibits the same excellent electron-recoil and alpha decay rejection as was previously reported. These data provide the most stringent direct detection constraints on weakly interacting massive particle (WIMP)-proton spin-dependent scattering to date for WIMP masses < 50 GeV/c(2).
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Copyrigths:
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Reserva de todos los derechos
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Source:
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Physical Review D. (issn:
2470-0010
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DOI:
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10.1103/PhysRevD.93.061101
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Publisher:
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American Physical Society
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Publisher version:
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http://dx.doi.org/10.1103/PhysRevD.93.061101
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Project ID:
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info:eu-repo/grantAgreement/NSF/Directorate for Mathematical & Physical Sciences/0919526/US/
...[+]
info:eu-repo/grantAgreement/NSF/Directorate for Mathematical & Physical Sciences/0919526/US/
info:eu-repo/grantAgreement/Fermilab//DE-AC02-07CH11359/
info:eu-repo/grantAgreement/NSF/Directorate for Mathematical & Physical Sciences/1242637/US/
info:eu-repo/grantAgreement/NSF//1506377/US/RUI: A Search For Dark Matter With Superheated Liquid Targets/
info:eu-repo/grantAgreement/NSF/Directorate for Mathematical & Physical Sciences/1205987/US/
info:eu-repo/grantAgreement/NSF//1242637/US/Construction of the COUPP-500kg Bubble Chamber for Dark Matter Detection/
info:eu-repo/grantAgreement/NSF//1205987/US/RUI: Searching for WIMP Dark Matter With Superheated Liquids/
info:eu-repo/grantAgreement/NSF//0919526/US/COUPP-500 kg: Design of a large-Mass Bubble Chamber for Dark Matter Detection/
info:eu-repo/grantAgreement/DOE//DE-SC-0012161/
info:eu-repo/grantAgreement/MSMT//LM2011027/
info:eu-repo/grantAgreement/MICINN//CSD2009-00064/ES/Método de Multimensajeros para la Detección de la Materia Oscura/
info:eu-repo/grantAgreement/UNAM//IA100316/MX/Búsqueda de materia oscura con los experimentos PICO y DEAP/
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Thanks:
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The PICO Collaboration thanks SNOLAB for their exceptional laboratory space and technical support. We also thank Fermi National Accelerator Laboratory (Contract No. DE-AC02-07CH11359) and Pacific Northwest National Laboratory ...[+]
The PICO Collaboration thanks SNOLAB for their exceptional laboratory space and technical support. We also thank Fermi National Accelerator Laboratory (Contract No. DE-AC02-07CH11359) and Pacific Northwest National Laboratory for their support. This work is supported by the National Sciences and Engineering Research Council of Canada (NSERC), the Canada Foundation for Innovation (CFI), the National Science Foundation (NSF) under the Grants No. PHY-1242637, No. PHY-0919526, No. PHY-1205987, and No. PHY-1506377 and by the U.S. Department of Energy under Award No. DE-SC-0012161. We also acknowledge the support of Department of Atomic Energy (DAE), Government of India, under the Center of AstroParticle Physics II project (CAPP-II) at Saha Institute of Physics (SINP); the Czech Ministry of Education, Youth and Sports (Grant No. LM2011027); the Spanish Ministerio de Economia y Competitividad, Consolider MultiDark (Grant No. CSD2009-00064) and DGAPA-UNAM through grant PAPIIT No. IA100316.
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Type:
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Artículo
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