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Dark matter search results from the PICO-60 CF3I bubble chamber

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Dark matter search results from the PICO-60 CF3I bubble chamber

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Nombre: PhysRevD.93.05201 ...
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dc.contributor.author Amole, C. es_ES
dc.contributor.author Ardid Ramírez, Miguel es_ES
dc.contributor.author Asner, D. M. es_ES
dc.contributor.author Baxter, D. es_ES
dc.contributor.author Behnke, E. es_ES
dc.contributor.author Bhattacharjee, P. es_ES
dc.contributor.author Borsodi, H. es_ES
dc.contributor.author Bou Cabo, Manuel es_ES
dc.contributor.author Brice, S. J. es_ES
dc.contributor.author Broemmelsiek, D. es_ES
dc.contributor.author Clark, K. es_ES
dc.contributor.author Collar, J. I. es_ES
dc.contributor.author Cooper, P. S. es_ES
dc.contributor.author Crisler, M. es_ES
dc.contributor.author Felis Enguix, Iván es_ES
dc.date.accessioned 2017-05-02T10:34:47Z
dc.date.available 2017-05-02T10:34:47Z
dc.date.issued 2016-03-28
dc.identifier.issn 2470-0010
dc.identifier.uri http://hdl.handle.net/10251/80310
dc.description.abstract New data are reported from the operation of the PICO-60 dark matter detector, a bubble chamber filled with 36.8 kg of CF3I and located in the SNOLAB underground laboratory. PICO-60 is the largest bubble chamber to search for dark matter to date. With an analyzed exposure of 92.8 livedays, PICO-60 exhibits the same excellent background rejection observed in smaller bubble chambers. Alpha decays in PICO-60 exhibit frequency-dependent acoustic calorimetry, similar but not identical to that reported recently in a C3F8 bubble chamber. PICO-60 also observes a large population of unknown background events, exhibiting acoustic, spatial, and timing behaviors inconsistent with those expected from a dark matter signal. These behaviors allow for analysis cuts to remove all background events while retaining 48.2% of the exposure. Stringent limits on weakly interacting massive particles interacting via spin-dependent proton and spin-independent processes are set, and most interpretations of the DAMA/LIBRA modulation signal as dark matter interacting with iodine nuclei are ruled out. es_ES
dc.description.sponsorship The PICO Collaboration would like to thank SNOLAB and its staff for providing an exceptional underground laboratory space and invaluable technical support. We acknowledge technical assistance from Fermilab's Computing, Particle Physics, and Accelerator Divisions and from A. Behnke at IUSB. We thank V. Gluscevic and S. McDermott for useful conversations and their assistance with the DMDD code package. This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of High Energy Physics under Award No. DE-SC-0012161. Fermi National Accelerator Laboratory is operated by Fermi Research Alliance, LLC under Contract No. De-AC02-07CH11359. Part of the research described in this paper was conducted under the Ultra Sensitive Nuclear Measurements Initiative at Pacific Northwest National Laboratory, a multiprogram national laboratory operated by Battelle for the U.S. Department of Energy. We acknowledge the National Science Foundation for their support including Grants No. PHY-1242637, No. PHY-0919526, and No. PHY-1205987. We acknowledge the support of the National Sciences and Engineering Research Council of Canada (NSERC) and the Canada Foundation for Innovation (CFI). We thank the Kavli Institute for Cosmological Physics at the University of Chicago. We were also supported by the Spanish Ministerio de Economia y Competitividad, Consolider MultiDark CSD2009-00064 Grant. We thank the Department of Atomic Energy (DAE), Government of India, under the project CAPP-II at SINP, Kolkata. We acknowledge the Czech Ministry of Education, Youth and Sports, Grant No. LM2011027. en_EN
dc.language Inglés es_ES
dc.publisher American Physical Society es_ES
dc.relation.ispartof Physical Review D es_ES
dc.rights Reserva de todos los derechos es_ES
dc.subject.classification FISICA APLICADA es_ES
dc.title Dark matter search results from the PICO-60 CF3I bubble chamber es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1103/PhysRevD.93.052014
dc.relation.projectID info:eu-repo/grantAgreement/DOE//DE-SC-0012161/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NSF/Directorate for Mathematical & Physical Sciences/0919526/US/ en_EN
dc.relation.projectID info:eu-repo/grantAgreement/NSF/Directorate for Mathematical & Physical Sciences/1242637/US/
dc.relation.projectID info:eu-repo/grantAgreement/Fermilab//DE-AC02-07CH11359/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NSF/Directorate for Mathematical & Physical Sciences/1205987/US/
dc.relation.projectID info:eu-repo/grantAgreement/NSF//1242637/US/Construction of the COUPP-500kg Bubble Chamber for Dark Matter Detection/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NSF//1205987/US/RUI: Searching for WIMP Dark Matter With Superheated Liquids/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NSF//0919526/US/COUPP-500 kg: Design of a large-Mass Bubble Chamber for Dark Matter Detection/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MICINN//CSD2009-00064/ES/Método de Multimensajeros para la Detección de la Materia Oscura/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MSMT//LM2011027/ es_ES
dc.rights.accessRights Abierto es_ES
dc.contributor.affiliation 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 es_ES
dc.contributor.affiliation Universitat Politècnica de València. Escuela Técnica Superior de Ingeniería del Diseño - Escola Tècnica Superior d'Enginyeria del Disseny es_ES
dc.description.bibliographicCitation Amole, C.; Ardid Ramírez, M.; Asner, DM.; Baxter, D.; Behnke, E.; Bhattacharjee, P.; Borsodi, H.... (2016). Dark matter search results from the PICO-60 CF3I bubble chamber. Physical Review D. 93(5):1-14. https://doi.org/10.1103/PhysRevD.93.052014 es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion http://dx.doi.org/10.1103/PhysRevD.93.052014 es_ES
dc.description.upvformatpinicio 1 es_ES
dc.description.upvformatpfin 14 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 93 es_ES
dc.description.issue 5 es_ES
dc.relation.senia 320192 es_ES
dc.contributor.funder Ministerio de Ciencia e Innovación es_ES
dc.contributor.funder Fermilab es_ES
dc.contributor.funder National Science Foundation, EEUU es_ES
dc.contributor.funder Ministry of Education, Youth and Sports, República Checa es_ES
dc.contributor.funder U.S. Department of Energy es_ES
dc.contributor.funder Canada Foundation for Innovation es_ES
dc.contributor.funder Department of Atomic Energy, Government of India es_ES
dc.contributor.funder Natural Sciences and Engineering Research Council of Canada es_ES
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