PICASSO, COUPP and PICO - search for dark matter with bubble chambers

PICASSO, COUPP and PICO - search for dark matter with bubble chambers

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The PICASSO and COUPP collaborations use superheated liquid detectors to search for cold dark matter through the direct detection of weakly interacting massive particles (WIMPs). These experiments, located in the underground laboratory of SNOLAB, Canada, detect phase transitions triggered by nuclear...

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Main Authors: Amole C., Ardid M., Asner D. M., Baxter D., Behnke E., Bhattacharjee P., Borsodi H., Bou-Cabo M., Brice S. J., Broemmelsiek D., Clark K., Collar J. I., Cooper P. S., Crisler M., Dahl C. E., Das M., Debris F., Dhungana N., Farine J., Felis I., Filgas R., Fines-Neuschild M., Girard F., Giroux G., Hai M., Hall J., Harris O., Jackson C. M., Jin M., Krauss C., Lafrenière M., Laurin M., Lawson I., Levine I., Lippincott W. H., Mann E., Martin J. P., Maurya D., Mitra P., Neilson R., Noble A. J., Plante A., Podviyanuk R., Priya S., Robinson A. E., Ruschman M., Scallon O., Seth S., Sonnenschein A., Starinski N., Štekl I., Vázquez-Jáuregui E., Wells J., Wichoski U., Zacek V., Zhang J.
Format: Article
Language:English
Published: EDP Sciences 2015-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20159504020
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author Amole C.
Ardid M.
Asner D. M.
Baxter D.
Behnke E.
Bhattacharjee P.
Borsodi H.
Bou-Cabo M.
Brice S. J.
Broemmelsiek D.
Clark K.
Collar J. I.
Cooper P. S.
Crisler M.
Dahl C. E.
Das M.
Debris F.
Dhungana N.
Farine J.
Felis I.
Filgas R.
Fines-Neuschild M.
Girard F.
Giroux G.
Hai M.
Hall J.
Harris O.
Jackson C. M.
Jin M.
Krauss C.
Lafrenière M.
Laurin M.
Lawson I.
Levine I.
Lippincott W. H.
Mann E.
Martin J. P.
Maurya D.
Mitra P.
Neilson R.
Noble A. J.
Plante A.
Podviyanuk R.
Priya S.
Robinson A. E.
Ruschman M.
Scallon O.
Seth S.
Sonnenschein A.
Starinski N.
Štekl I.
Vázquez-Jáuregui E.
Wells J.
Wichoski U.
Zacek V.
Zhang J.
spellingShingle Amole C.
Ardid M.
Asner D. M.
Baxter D.
Behnke E.
Bhattacharjee P.
Borsodi H.
Bou-Cabo M.
Brice S. J.
Broemmelsiek D.
Clark K.
Collar J. I.
Cooper P. S.
Crisler M.
Dahl C. E.
Das M.
Debris F.
Dhungana N.
Farine J.
Felis I.
Filgas R.
Fines-Neuschild M.
Girard F.
Giroux G.
Hai M.
Hall J.
Harris O.
Jackson C. M.
Jin M.
Krauss C.
Lafrenière M.
Laurin M.
Lawson I.
Levine I.
Lippincott W. H.
Mann E.
Martin J. P.
Maurya D.
Mitra P.
Neilson R.
Noble A. J.
Plante A.
Podviyanuk R.
Priya S.
Robinson A. E.
Ruschman M.
Scallon O.
Seth S.
Sonnenschein A.
Starinski N.
Štekl I.
Vázquez-Jáuregui E.
Wells J.
Wichoski U.
Zacek V.
Zhang J.
PICASSO, COUPP and PICO - search for dark matter with bubble chambers
EPJ Web of Conferences
author_facet Amole C.
Ardid M.
Asner D. M.
Baxter D.
Behnke E.
Bhattacharjee P.
Borsodi H.
Bou-Cabo M.
Brice S. J.
Broemmelsiek D.
Clark K.
Collar J. I.
Cooper P. S.
Crisler M.
Dahl C. E.
Das M.
Debris F.
Dhungana N.
Farine J.
Felis I.
Filgas R.
Fines-Neuschild M.
Girard F.
Giroux G.
Hai M.
Hall J.
Harris O.
Jackson C. M.
Jin M.
Krauss C.
Lafrenière M.
Laurin M.
Lawson I.
Levine I.
Lippincott W. H.
Mann E.
Martin J. P.
Maurya D.
Mitra P.
Neilson R.
Noble A. J.
Plante A.
Podviyanuk R.
Priya S.
Robinson A. E.
Ruschman M.
Scallon O.
Seth S.
Sonnenschein A.
Starinski N.
Štekl I.
Vázquez-Jáuregui E.
Wells J.
Wichoski U.
Zacek V.
Zhang J.
author_sort Amole C.
title PICASSO, COUPP and PICO - search for dark matter with bubble chambers
title_short PICASSO, COUPP and PICO - search for dark matter with bubble chambers
title_full PICASSO, COUPP and PICO - search for dark matter with bubble chambers
title_fullStr PICASSO, COUPP and PICO - search for dark matter with bubble chambers
title_full_unstemmed PICASSO, COUPP and PICO - search for dark matter with bubble chambers
title_sort picasso, coupp and pico - search for dark matter with bubble chambers
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2015-01-01
description The PICASSO and COUPP collaborations use superheated liquid detectors to search for cold dark matter through the direct detection of weakly interacting massive particles (WIMPs). These experiments, located in the underground laboratory of SNOLAB, Canada, detect phase transitions triggered by nuclear recoils in the keV range induced by interactions with WIMPs. We present details of the construction and operation of these detectors as well as the results, obtained by several years of observations. We also introduce PICO, a joint effort of the two collaborations to build a second generation ton-scale bubble chamber with 250 liters of active liquid.
url http://dx.doi.org/10.1051/epjconf/20159504020
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spelling doaj-02ba95d33d674d3f8d8c2f6282d714a32021-08-02T05:39:03ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-01950402010.1051/epjconf/20159504020epjconf_icnfp2014_04020PICASSO, COUPP and PICO - search for dark matter with bubble chambersAmole C.0Ardid M.1Asner D. M.2Baxter D.3Behnke E.4Bhattacharjee P.5Borsodi H.6Bou-Cabo M.7Brice S. J.8Broemmelsiek D.9Clark K.10Collar J. I.11Cooper P. S.12Crisler M.13Dahl C. E.14Das M.15Debris F.16Dhungana N.17Farine J.18Felis I.19Filgas R.20Fines-Neuschild M.21Girard F.22Giroux G.23Hai M.24Hall J.25Harris O.26Jackson C. M.27Jin M.28Krauss C.29Lafrenière M.30Laurin M.31Lawson I.Levine I.32Lippincott W. H.33Mann E.34Martin J. P.35Maurya D.36Mitra P.37Neilson R.Noble A. J.38Plante A.39Podviyanuk R.40Priya S.41Robinson A. E.42Ruschman M.43Scallon O.Seth S.44Sonnenschein A.45Starinski N.46Štekl I.47Vázquez-Jáuregui E.Wells J.48Wichoski U.49Zacek V.50Zhang J.51Department of Physics, Queen’s UniversityUniversitat Politècnica de València, IGICPacific Northwest National LaboratoryDepartment of Physics, Northwestern UniversityDepartment of Physics, Indiana University South Bend, South BendAstroparticle Physics and Cosmology Division, Saha Institute of Nuclear PhysicsDepartment of Physics, Indiana University South Bend, South BendUniversitat Politècnica de València, IGICFermi National Accelerator LaboratoryFermi National Accelerator LaboratoryDepartment of Physics, University of TorontoEnrico Fermi Institute, KICP and Department of Physics, University of ChicagoFermi National Accelerator LaboratoryFermi National Accelerator LaboratoryDepartment of Physics, Northwestern UniversityAstroparticle Physics and Cosmology Division, Saha Institute of Nuclear PhysicsDépartement de Physique, Université de MontréalDepartment of Physics, Laurentian UniversityDepartment of Physics, Laurentian UniversityUniversitat Politècnica de València, IGICInstitute of Experimental and Applied Physics, Czech Technical University in PragueDépartement de Physique, Université de MontréalDépartement de Physique, Université de MontréalDepartment of Physics, Queen’s UniversityEnrico Fermi Institute, KICP and Department of Physics, University of ChicagoPacific Northwest National LaboratoryDepartment of Physics, Indiana University South Bend, South BendDépartement de Physique, Université de MontréalDepartment of Physics, Northwestern UniversityDepartment of Physics, University of AlbertaDépartement de Physique, Université de MontréalDépartement de Physique, Université de MontréalDepartment of Physics, Indiana University South Bend, South BendFermi National Accelerator LaboratoryDepartment of Physics, Indiana University South Bend, South BendDépartement de Physique, Université de MontréalCenter for Intelligent Material Systems and Structures, Virginia TechDepartment of Physics, University of AlbertaDepartment of Physics, Queen’s UniversityDépartement de Physique, Université de MontréalDepartment of Physics, Laurentian UniversityCenter for Intelligent Material Systems and Structures, Virginia TechEnrico Fermi Institute, KICP and Department of Physics, University of ChicagoFermi National Accelerator LaboratoryAstroparticle Physics and Cosmology Division, Saha Institute of Nuclear PhysicsFermi National Accelerator LaboratoryDépartement de Physique, Université de MontréalInstitute of Experimental and Applied Physics, Czech Technical University in PragueDepartment of Physics, Indiana University South Bend, South BendDepartment of Physics, Laurentian UniversityDépartement de Physique, Université de MontréalDepartment of Physics, Northwestern UniversityThe PICASSO and COUPP collaborations use superheated liquid detectors to search for cold dark matter through the direct detection of weakly interacting massive particles (WIMPs). These experiments, located in the underground laboratory of SNOLAB, Canada, detect phase transitions triggered by nuclear recoils in the keV range induced by interactions with WIMPs. We present details of the construction and operation of these detectors as well as the results, obtained by several years of observations. We also introduce PICO, a joint effort of the two collaborations to build a second generation ton-scale bubble chamber with 250 liters of active liquid.http://dx.doi.org/10.1051/epjconf/20159504020

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