Show simple item record

dc.contributor.authorRielage, K.
dc.contributor.authorAkashi-Ronquest, M.
dc.contributor.authorBodmer, M.
dc.contributor.authorBourque, R.
dc.contributor.authorButcher, A.
dc.contributor.authorCaldwell, T.
dc.contributor.authorChen, Y.
dc.contributor.authorCoakley, K.
dc.contributor.authorFlores, E.
dc.contributor.authorGastler, D.
dc.contributor.authorGiuliani, F.
dc.contributor.authorGold, M.
dc.contributor.authorGrace, E.
dc.contributor.authorGriego, J.
dc.contributor.authorGuiseppe, V.
dc.contributor.authorHenning, R.
dc.contributor.authorHime, A.
dc.contributor.authorKachulis, C.
dc.contributor.authorKearns, E.
dc.contributor.authorKlein, J.R.
dc.contributor.authorLatorre, A.
dc.contributor.authorLawson, I.
dc.contributor.authorLinden, S.
dc.contributor.authorLopez, F.
dc.contributor.authorMcKinsey, D.N.
dc.contributor.authorMacMullin, S.
dc.contributor.authorMastbaum, A.
dc.contributor.authorMei, D.-M.
dc.contributor.authorMonroe, J.
dc.contributor.authorNikkel, J.A.
dc.contributor.authorOertel, J.
dc.contributor.authorOrebi Gann, G.D.
dc.contributor.authorPalladino, K.
dc.contributor.authorPerumpilly, G.
dc.contributor.authorRodriguez, L.
dc.contributor.authorSchnee, R.
dc.contributor.authorSeibert, S.
dc.contributor.authorWalding, J.
dc.contributor.authorWang, B.
dc.contributor.authorWang, J.
dc.contributor.authorZhang, C.
dc.contributor.authorBuck, Benjamin R.
dc.contributor.authorFormaggio, Joseph A
dc.contributor.authorKelsey, James E
dc.contributor.authorGuerrero, Natalia M.
dc.date.accessioned2017-04-19T14:32:27Z
dc.date.available2017-04-19T14:32:27Z
dc.date.issued2015-03
dc.identifier.issn1875-3892
dc.identifier.urihttp://hdl.handle.net/1721.1/108244
dc.description.abstractThe direct search for dark matter is entering a period of increased sensitivity to the hypothetical Weakly Interacting Massive Particle (WIMP). One such technology that is being examined is a scintillation only noble liquid experiment, MiniCLEAN. MiniCLEAN utilizes over 500 kg of liquid cryogen to detect nuclear recoils from WIMP dark matter and serves as a demonstration for a future detector of order 50 to 100 tonnes. The liquid cryogen is interchangeable between argon and neon to study the A2 dependence of the potential signal and examine backgrounds. MiniCLEAN utilizes a unique modular design with spherical geometry to maximize the light yield using cold photomultiplier tubes in a single-phase detector. Pulse shape discrimination techniques are used to separate nuclear recoil signals from electron recoil backgrounds. MiniCLEAN will be spiked with additional 39Ar to demonstrate the effective reach of the pulse shape discrimination capability. Assembly of the experiment is underway at SNOLAB and an update on the project is given.en_US
dc.description.sponsorshipLos Alamos National Laboratoryen_US
dc.description.sponsorshipUnited States. Department of Energy. Office of Scienceen_US
dc.description.sponsorshipNational Science Foundation (U.S.)en_US
dc.description.sponsorshipNational Institute of Standards and Technology (U.S.)en_US
dc.language.isoen_US
dc.publisherElsevieren_US
dc.relation.isversionofhttp://dx.doi.org/10.1016/j.phpro.2014.12.024en_US
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivs Licenseen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/en_US
dc.sourceElsevieren_US
dc.titleUpdate on the MiniCLEAN Dark Matter Experimenten_US
dc.typeArticleen_US
dc.identifier.citationRielage, K.; Akashi-Ronquest, M.; Bodmer, M.; Bourque, R.; Buck, B.; Butcher, A.; Caldwell, T. et al. “Update on the MiniCLEAN Dark Matter Experiment.” Physics Procedia 61 (2015): 144–152. © Elsevier B.V.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorBuck, Benjamin R.
dc.contributor.mitauthorFormaggio, Joseph A
dc.contributor.mitauthorKelsey, James E
dc.contributor.mitauthorGuerrero, Natalia M.
dc.relation.journalPhysics Procediaen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsRielage, K.; Akashi-Ronquest, M.; Bodmer, M.; Bourque, R.; Buck, B.; Butcher, A.; Caldwell, T.; Chen, Y.; Coakley, K.; Flores, E.; Formaggio, J.A.; Gastler, D.; Giuliani, F.; Gold, M.; Grace, E.; Griego, J.; Guerrero, N.; Guiseppe, V.; Henning, R.; Hime, A.; Jaditz, S.; Kachulis, C.; Kearns, E.; Kelsey, J.; Klein, J.R.; Latorre, A.; Lawson, I.; Linden, S.; Lopez, F.; McKinsey, D.N.; MacMullin, S.; Mastbaum, A.; Mei, D.-M.; Monroe, J.; Nikkel, J.A.; Oertel, J.; Gann, G.D. Orebi; Palladino, K.; Perumpilly, G.; Rodriguez, L.; Schnee, R.; Seibert, S.; Walding, J.; Wang, B.; Wang, J.; Zhang, C.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-3757-9883
mit.licensePUBLISHER_CCen_US


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record