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Dark Matter Search Results from the PICO-60C(3)F(8) Bubble Chamber

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Dark Matter Search Results from the PICO-60C(3)F(8) Bubble Chamber

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dc.contributor.author Amole, C. es_ES
dc.contributor.author Ardid Ramírez, Miguel es_ES
dc.contributor.author Arnquist, I.J. 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 Campion, P. es_ES
dc.contributor.author Cao, G. es_ES
dc.contributor.author Chen, C.J. es_ES
dc.contributor.author Chowdhury, U. es_ES
dc.contributor.author Clark, K. es_ES
dc.contributor.author Felis-Enguix, Iván es_ES
dc.date.accessioned 2020-04-24T07:13:02Z
dc.date.available 2020-04-24T07:13:02Z
dc.date.issued 2017 es_ES
dc.identifier.issn 0031-9007 es_ES
dc.identifier.uri http://hdl.handle.net/10251/141427
dc.description.abstract [EN] New results are reported from the operation of the PICO-60 dark matter detector, a bubble chamber filled with 52 kg of C3F8 located in the SNOLAB underground laboratory. As in previous PICO bubble chambers, PICO-60 C3F8 exhibits excellent electron recoil and alpha decay rejection, and the observed multiple-scattering neutron rate indicates a single-scatter neutron background of less than one event per month. A blind analysis of an efficiency-corrected 1167-kg day exposure at a 3.3-keV thermodynamic threshold reveals no single-scattering nuclear recoil candidates, consistent with the predicted background. These results set the most stringent direct-detection constraint to date on the weakly interacting massive particle (WIMP)-proton spin-dependent cross section at 3.4 x 10(-41) cm(2) for a 30-GeVc(-2) WIMP, more than 1 order of magnitude improvement from previous PICO results. es_ES
dc.description.sponsorship The PICO Collaboration wishes to thank SNOLAB and its staff for support through underground space, logistical, and technical services. SNOLAB operations are supported by the Canada Foundation for Innovation and the Province of Ontario Ministry of Research and Innovation, with underground access provided by Vale at the Creighton mine site. We are grateful to Kristian Hahn and Stanislava Sevova of Northwestern University and Bjorn Penning of the University of Bristol for their assistance and useful discussion. We wish to acknowledge the support of the Natural Sciences and Engineering Research Council of Canada (NSERC) and the Canada Foundation for Innovation (CFI) for funding. We acknowledge the support from National Science Foundation (NSF) (Grants No. 0919526, No. 1506337, No. 1242637, and No. 1205987). We acknowledge that this work is supported by the U.S. Department of Energy (DOE) Office of Science, Office of High Energy Physics (under Award No. DE-SC-0012161), by a DOE Office of Science Graduate Student Research (SCGSR) award, by Direccion General Asuntos del Personal Academico, Universidad Nacional Autonoma de Mexico (DGAPA-UNAM) through the grant Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPIIT) No. IA100316 and by Consejo Nacional de Ciencia y Tecnologia (CONACyT) (Mexico) through Grant No. 252167, by the Department of Atomic Energy (DAE), the Government of India, under the Center of AstroParticle Physics II project (CAPP-II) at Saha Institute of Nuclear Physics (SINP), by the Czech Ministry of Education, Youth and Sports (Grant No. LM2015072), and by the Spanish Ministerio de Economia y Competitividad, Consolider MultiDark (Grant No. CSD2009-00064). This work is partially supported by the Kavli Institute for Cosmological Physics at the University of Chicago through NSF Grant No. 1125897, and an endowment from the Kavli Foundation and its founder Fred Kavli. We also wish to acknowledge the support from Fermi National Accelerator Laboratory under Contract No. De-AC02-07CH11359, and Pacific Northwest National Laboratory, which is operated by Battelle for the U.S. Department of Energy under Contract No. DE-AC05-76RL01830. We also thank Compute Canada and the Center for Advanced Computing, ACENET, Calcul Quebec, Compute Ontario, and WestGrid for the computational support. es_ES
dc.language Inglés es_ES
dc.publisher American Physical Society es_ES
dc.relation.ispartof Physical Review Letters 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-60C(3)F(8) Bubble Chamber es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1103/PhysRevLett.118.251301 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/NSF//1506337/US/ es_ES
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/DOE//DE-SC-0012161/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/UNAM/PAPIIT/IA100316/MX/Búsqueda de materia oscura con los experimentos PICO y DEAP/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/CONACyT//252167/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MSMT//LM2015072/ 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.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. Departamento de Física Aplicada - Departament de Física Aplicada es_ES
dc.description.bibliographicCitation Amole, C.; Ardid Ramírez, M.; Arnquist, I.; Asner, DM.; Baxter, D.; Behnke, E.; Bhattacharjee, P.... (2017). Dark Matter Search Results from the PICO-60C(3)F(8) Bubble Chamber. Physical Review Letters. 118(25). https://doi.org/10.1103/PhysRevLett.118.251301 es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion https://doi.org/10.1103/PhysRevLett.118.251301 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 118 es_ES
dc.description.issue 25 es_ES
dc.relation.pasarela S\348307 es_ES
dc.contributor.funder U.S. Department of Energy es_ES
dc.contributor.funder Canada Foundation for Innovation es_ES
dc.contributor.funder National Science Foundation, EEUU es_ES
dc.contributor.funder Universidad Nacional Autónoma de México es_ES
dc.contributor.funder Ontario Ministry of Research and Innovation es_ES
dc.contributor.funder Ministry of Education, Youth and Sports, República Checa es_ES
dc.contributor.funder Department of Atomic Energy, Government of India es_ES
dc.contributor.funder Consejo Nacional de Ciencia y Tecnología, México es_ES
dc.contributor.funder Natural Sciences and Engineering Research Council of Canada es_ES
dc.contributor.funder Ministerio de Ciencia e Innovación es_ES
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